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Stellar astrophysics
The materials presented at the exhibition cover various aspects of modern astrophysics: questions of the life and origin of stars, physics and dynamics of stellar systems, characteristics of stars and the theory of their internal structure. The stages of stellar evolution leading to the formation of planetary nebulae, white dwarfs, neutron stars, as well as new and supernova outbreaks are discussed. Much attention is paid to priority areas of solar research: the main mechanisms of solar activity, solar flares and unsteady processes, the structure of the Sun's atmosphere, solar wind and interplanetary magnetic fields, modern physics of the solar corona, the study of energy particle flows, as well as processes in near-Earth space plasma.
The exhibition can be useful for researchers engaged in the study of the physics of stars and the Sun, graduate students and students of astrophysical specialties.
The exhibition is held as part of the All-Russian Science Festival "Science 0+". During the preparation of the exhibition, publications from the fund of the State Scientific and Technical Library of Russia were used: monographs, conference materials, collections of reports, educational and methodological literature, abstracts of dissertations, preprints, periodicals, publications from the scientific electronic library "eLIBRARY.RU ", from the electronic library systems "Lan", "ZNANIUM.COM ", IPR SMART digital educational resource, and also publications from the full-text database of the Springer publishing house.
The materials of the exhibition can be found in the lobby of the 2nd floor of the main building from August 29 to October 23, 2022. At the end of the exhibition period, you can pre-order the print edition you are interested in from the list by clicking the "ORDER" button. To order, authorization is required in the reader's Personal Account. You can work with publications in the reading room selected by you when placing an order.
If you have any questions about the use of printed publications presented at the exhibition, please call: 8(495) 698-93-07, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it. or in a chat on the main page of the library's website.
Authorization is required to read electronic publications presented at the exhibition. The terms of access can be found in your Personal Account in the section "Licensed resources".
Thematic sections of the exhibition:
1. A star as an object of research
2. Heliophysics (physics of the Sun)
1. A star as an object of research
1. Амнуэль, П. Р. Далекие маяки Вселенной : научно-популярное издание / П. Р. Амнуэль. – Москва : ДМК Пресс, 2022. – 288 с. – ISBN 978-5-89818-200-7. – URL: https://znanium.com/catalog/product/1870681 (дата обращения: 05.07.2022). – Access mode: for authorized users. – Text : electronic.
Abstract: The 50th anniversary of the discovery of the first pulsar has recently been celebrated. The history of the discovery of pulsars is full of drama. This is a story of great insights and deep delusions, amazing predictions and strange mistakes. The book tells about how scientists' ideas about the origin of stars, their life and death have changed over the centuries. About how neutron stars were predicted and how pulsars – "distant beacons of the universe" - were discovered. Using the example of this story, it is told about how discoveries are made in science, whether discoveries can be predicted, what is scientific imagination, how to develop creative imagination.
2. Д8-91/6373
Астрономо-геодезические исследования. Физика и динамика звездных систем : Сборник научных трудов / Уральский государственный университет имени А. М. Горького ; редакционная коллегия : А. Е. Василевский (ответственный редактор) [и др.]. – Свердловск, 1991. – 203 с. : ХУII с. : ил. – ISBN 5-230-06671-7. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The collection contains scientific works of employees of the Leningrad, Ural, Chelyabinsk, Mordovian Universities, the Astrophysical Institute of the Academy of Sciences of the Kazakh SSR, the Sverdlovsk Pedagogical Institute and is devoted to the study of physics and dynamics of stellar systems. A significant place in it is devoted to the results of numerical modeling in various fields of astrophysics, as well as research methods of astronomical observations and their mathematical processing.
3. Ж2-13/56142
Васильев, Б. В. Астрофизика с точки зрения физика / Б. В. Васильев. – Москва : Книга по Требованию, 2013. – 127 с. – Библиогр.: с. 119-127 (85 назв.). – ISBN 978-5-458-62593-7. – Текст : непосредственный.
Abstract: The modern astrophysical community bases research on the physics of stars on the principle of their internal consistency and consistency with the main provisions of previously accumulated theories and models. This is the fundamental difference between modern astrophysics and other branches of physics, which base their developments on their agreement with measurement data. To date, astronomers have measured a number of dependencies and parameters of stars, which can serve as a reliable foundation for constructing a theory of their internal structure. In order to reach agreement between the theory and the available astronomical measurement data, it turns out to be necessary to abandon some astrophysical constructions that are generally accepted today. First of all, we need to change the approach to describing the equilibrium of matter inside stars. It should be taken into account that the interior of stars is plasma – an electrically polarizable medium. Therefore, the equilibrium equation of interstellar matter must take into account the role of gravitationally induced electric polarization. Taking into account the gravitationally induced electric polarization of the intrastellar plasma allows us to build a model of a star in which all the main parameters - the mass of the star, its temperature, radius and luminosity – are expressed by certain combinations of world constants, and the individuality of stars is determined only by two parameters – the mass and charge numbers of atomic nuclei, from which the plasma of these stars is built. At the same time, it is possible to explain quantitatively and with satisfactory accuracy all the dependencies measured by astronomers. Taking into account the gravitationally induced polarization, theories of rotation of the periasters of close binary stars and magnetic fields of stars are constructed, consistent with the observational data. It is important to note that taking into account gravitationally induced polarization leads to other conceptual changes, for example, it rejects the mechanism of collapse of stars at the last stage of their evolution and thereby denies the possibility of the formation of "black holes" as a result of collapse. As a result of this restructuring, the physics of stars receives a reliable foundation in the form of measurement data, on which physical science should be built.
4. Н/8977/Пр-1982
Витриченко, Э. А. Пылевые оболочки вокруг спутников звезд ВМ Ori и V1016 Ori / Э. А. Витриченко. – Москва, 1998. – 24 с. : ил. – (Препринт / Институт космических исследований (Москва) ; Пр-1982). – Текст : непосредственный.
Abstract: The question of the possibility of the survival of dust shells around the satellites of B-stars VM Ori b V1016 Ori has been studied. It is shown that the assumption of the existence of shells is inevitable.
5. Д7-90/71415
Вопросы небесной механики и звездной динамики : сборник статей / редакционная коллегия : Т. Б. Омаров (ответственный редактор) [и др.]. – Алма-Ата : Наука КазССР, 1990. – 207 c. : ил. – ISBN 5-628-00162-7. – В надзаг.: АН КазССР, Астрофиз. ин-т им. В. Г. Фесенкова. – Библиогр. в конце докл. – Текст : непосредственный.
Abstract: The materials of the All-Union Meeting "Dynamics of Gravitating systems and methods of analytical celestial mechanics", which make up this collection, contain works devoted to theoretical studies of structural and dynamic features of gravitating Metagalactic systems by modern methods of celestial mechanics, physical kinetics, theory of dynamical systems and relativistic dynamics. The collection is intended for astronomers, mechanics and physicists.
6. М/14715/1479
Городинский, Г. М. О дефекте массы нейтронной звезды / Г. М. Городинский, А. Ю. Добин, С. В. Бобышев. – Ленинград, 1990. – 17 с. : ил. – (Препринт / Физико-техн. ин-т им. А. Ф. Иоффе (Ленинград) ; 1479). – Библиогр.: с. 17 (6 назв.). – Текст : непосредственный.
Abstract: The total mass of a neutron star is determined as a function of the sum of the masses of its constituent particles, in the classical and relativistic cases.
7. М/42146/115/1
Госачинский, И. В. Распределение нейтрального водорода в области звездных ассоциаций Лебедь ОВ1-ОВ3 с высоким угловым разрешением. Крупномасштабная структура / И. В. Госачинский, Т. А. Лозинская. – Санкт-Петербург : [б. и.], 1995. – 33 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 115). – Текст : непосредственный.
Abstract: According to HI observations on the RATAN-600 radio telescope, the presence of a ring structure of neutral hydrogen in the region of the Cygnus 0B1 stellar association at positive radial velocities has been confirmed and it is shown that no traces of radial gas movements in it are imperceptible. In the region of the Swan-X radio source, a connection was found between the distribution of HI and the huge shell previously detected by Ha fibers, as well as with the distribution of ionized gas along recombination lines.
8. Д7-90/82594
Гоффмейстер, К. Переменные звезды / К. Гоффмейстер, Г. Рихтер, В. Вецель ; перевод с немецкого А. Г. Тоточава, Э. И. Желвановой ; под редакцией Н. Н. Самуся. – Москва : Наука, 1990. – 359 с. : ил. – Пер. изд.: Veranderliche Sterne / C. Hoffmeister, R. Richter, W. Wenzel. – Leipzig, 1990. – ISBN 5-02-014352-9. – Библиогр.: с. 337-359. – Текст : непосредственный.
Abstract: The problem that constantly occupies one of the central places in stellar astronomy, the study of variable stars, is comprehensively covered. All the main types of variable stars are considered, with special attention to their evolutionary status, the physical causes of variability, the connection of studies of variable stars with the problems of studying the structure of the Galaxy. This edition has been revised taking into account the latest data by well-known specialists G. Richter and V. Wenzel. The book is distinguished by a clear presentation of the material and scientific rigor. For students of astronomical specialties and astronomy specialists working both directly in the field of stellar variability research and in related fields, as well as astronomy enthusiasts.
9. М/51658/207
Грязных, Д. А. Структура термоядерной детонации в гелии / Д. А. Грязных. – Снежинск, 2004. – 28 с. : ил. – (Препринт / Всероссийский НИИ технической физики (Челябинск) ; 207). – Библиогр.: с. 28 (14 назв.). – Текст : непосредственный.
Abstract: The paper considers the parameters of thermonuclear detonation in helium. For a neat equation of state and a detailed set of isotopes and reactions, detonation adiabates of helium are obtained. A reduced set of isotopes has been analyzed, which makes it possible to reproduce detonation parameters fairly accurately. The influence of the equilibrium stat requirement in the final state is taken into account. The spatial structure of the Chapman-Jouguet thermonuclear detonation wave in helium during its combustion in the 3α–reaction and in (α, γ) –captures, and in further relaxation to the state of equilibrium is constructed. Gorenje The dependences of the Chapman-Jouget detonation parameters in helium on the initial density are found.
10. Данилов, В. М. Нестационарность рассеянных звездных скоплений : монография / В. М. Данилов. – Екатеринбург : Уральский федеральный университет, ЭБС АСВ, 2015. – 484 c. – ISBN 978-5-7996-1636-6. – URL: https://www.iprbookshop.ru/66557.html (дата обращения: 05.07.2022). – Access mode: for authorized users. – Text : electronic.
Abstract: The monograph consistently presents issues related to the study of the nonstationarity of scattered star clusters, starting with the analysis of the properties of the trajectories of single stars to the analysis of collective movements of stars, discussing the dynamics of correlations and wave processes in such clusters. The astrophysical applications of the results of studying the dynamics of the RSL are considered. The book contains formulas, tables, figures and can be used for research work in the field of dynamics of stellar systems. For researchers – astronomers and physicists interested in astrophysics and dynamics of stellar systems, graduate students and undergraduates of relevant specialties.
11. Ар18-2185
Дворников, М. С. Сильные магнитные поля в физике нейтрино, космологии и астрофизике : специальность 01.04.02 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Дворников М. С. – Москва, 2017. – 24 с. : ил. – Библиогр.: с. 22-24 (32 назв.). – Текст : непосредственный.
12. Д9-10/76349
Динамика тройных систем : учебное пособие / А. И. Мартынова [и др.]. – Санкт-Петербург : Изд-во С.-Петерб. ун-та, 2010 (СПб.). – 214 с. : ил. – Библиогр.: с. 200-214 (232 назв.). – ISBN 978-5-288-05041-1. – В надзаг.: С.-Петерб. гос. ун-т. – Текст : непосредственный.
Abstract: The book highlights various aspects of the gravitational problem of three bodies. The solution of this problem is the study of the dynamics of many astronomical objects, from triple stars and planetary systems to triplets of galaxies. The basic numerical and analytical methods for solving the three–body problem are described, depending on its features - the specifics of the initial conditions, the type and characteristics of objects and their surroundings, as well as other factors. The main results obtained by these methods are described. Much attention is paid to the issue of stability of triple systems. The presentation is accompanied by numerous illustrations. The book contains an extensive list of literature that the reader can use for a more detailed study of the side of the problem that interests him. Some of the results were obtained at the Department of Celestial Mechanics of St. Petersburg State University. For students and postgraduates of astronomical departments and departments of universities, as well as specialists in the field of stellar dynamics and celestial mechanics.
13. Дмитриев, Д. В. Модели магнитосферной аккреции на молодые звезды в отсутствие ионизационного равновесия / Д. В. Дмитриев, В. П. Гринин. – Text : electronic // Письма в Астрономический журнал. – 2022. – №1. – С. 34-42. – ISSN: 0320-0108. – URL: https://elibrary.ru/item.asp?id=47988448 (дата обращения: 05.07.2022). – Access mode: Scientific Electronic Library eLIBRARY.RU.
Abstract: The formation of hydrogen emission lines in the magnetospheres of young stars is considered. It is assumed that the magnetosphere is formed by a dipole magnetic field, the axis of which coincides with the axis of rotation of the star. The transfer of radiation in spectral lines is considered in the Sobolev approximation, taking into account the nonlocal radiation interaction. The effect of transferring the degree of gas ionization during motion in the magnetosphere is taken into account, its effect on the emission spectrum of the magnetosphere and estimates of the accretion rate along the Ha line are demonstrated for the first time.It is shown that at low accretion rates of M≲10-9 M⊙/year, this effect can have a significant impact on the model intensities.
14. М/42146/80 SP
Дубрович, В. К. Radio absorption by HeH+ molecules in spectra of the remote QSOs / В. К. Дубрович, А. А. Липовка. – Saint-Petersburg : [s. n.], 1992. – 15 p. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 80 SP). – Текст : непосредственный.
Abstract: The optical thickness in the lines of the rotational structure of the HeH+ molecule formed in Lyman-alpha clouds is calculated. The possibility of using a forest of absorption lines of the Hf+ molecule to determine the magnitude of the redshift of distant objects that do not have optical spectral lines is emphasized.
15. Н/13643/459
Железняков, В. В. Критическая температура белых карликов с сильным магнитным полем / В. В. Железняков, С. А. Корягин, А. В. Сербер. – Нижний Новгород, 1998. – 15 с. : ил. – (Препринт / Институт прикладной физики (Нижний Новгород) ; 459). – Текст : непосредственный.
Abstract: The cyclotron radiation pressure force in the plane-parallel isothermal hydrogen atmosphere of a white dwarf with a dipole magnetic field is calculated, taking into account the correct expressions for the frequency of collisions in the plasma on these stars. It is shown that a significant decrease in the frequency of collisions in a strong magnetic field leads to an increase in the critical temperature of magnetic white dwarfs, at which the force of radiation pressure is compared with the force of gravity acting on the proton. This means that the formation of plasma shells in the magnetospheres of candidates for radiation disks – magnetic white dwarfs GD 229, PG 1031 + 234 and GrW + 70o 8247 due to plasma injection from the photosphere requires a positive temperature gradient in its upper layers.
16. Н/13643/435
Железняков, В. В. Электрон-протонные столкновения в плазме на магнитных белых карликах / В. В. Железняков, С. А. Корягин, А. В. Сербер. – Нижний Новгород, 1997. – 15 с. : ил. – (Препринт/ Институт прикладной физики (Нижний Новгород) ; 435). – Текст : непосредственный.
Abstract: The electron motion in a homogeneous magnetic field of a proton is analyzed under conditions when the Larmor radius of the electron is less than the characteristic sighting parameter of a collision with scattering at large angles; A new expression is obtained for the effective frequency of electron-proton collisions in the classical plasma of the iei.It is shown that in this case, which, in particular, is easily realized in the photospheres of magnetic white dwarfs, the known expressions for yei become inapplicable.This circumstance plays a very important role in the calculations of radiation transfer and the strength of radiation pressure in the photospheres of these stars.
17. Д9-08/54507
Звезды / В. П. Архипова [и др.] ; редактор-составитель В. Г. Сурдин. – Москва : Физматлит, 2008 (Калуга). – 427 с. – (Астрономия и астрофизика). – Библиогр. в конце глав. – ISBN 978-5-94052-164-8. – Текст : непосредственный.
Abstract: The third book in the series "Astronomy and Astrophysics" contains an overview of modern ideas about stars. It tells about the names of constellations and the names of stars, about the possibility of observing them at night and during the day, about the main characteristics of stars and their classification. The main attention is paid to the nature of stars: their internal structure, energy sources, origin and evolution. The late stages of stellar evolution leading to the formation of planetary nebulae, white dwarfs, neutron stars, as well as the outbursts of new and supernovae are discussed. The book is aimed at undergraduate students of natural science faculties of universities and specialists in related fields of science. The book is of particular interest to fans of astronomy.
18. Зубко, О. Л. Релятивистские эффекты движения частицы в фотогравитационном поле звезды / О. Л. Зубко. – Text : electronic // Вестник БГУ. Серия 1. Физика. Математика. Информатика. – 2014. – № 3. – С. 30-33. – ISSN 1561-834X. – URL: https://e.lanbook.com/journal/issue/295544 (дата обращения: 05.07.2022). – Access mode: for authorized users.
Abstract: The relativistic motion of a particle in the photogravitational field of a star at different levels is considered. It is shown that when taking into account the direct light pressure, the elliptical orbit of the particle increases in size. Taking into account the longitudinal Doppler effect and the aberration of light leads to the movement of the particle along a decreasing ellipse, which also decreases the eccentricity.
19. Н/11110/97-91
Имшенник, В. С. Сверхновая 1987А и образование вращающихся нейтронных звезд / В. С. Имшенник, Д. К. Надежин. – Москва, 1991. – 30 с. – (Препринт / Институт теоретической и экспериментальной физики (Москва) ; 97-91). – Текст : непосредственный.
Abstract: The main characteristics of the neutrino signal from CH 1987A, such as its duration and the characteristic energy of the detected neutrinos, were in good agreement with the results of theoretical calculations of the gravitational collapse of massive stellar nuclei, which were performed long before the outbreak of CH 1987A in the approximation of spherical symmetry – without taking into account the effects of rotation and magnetic field.
20. Ж2-90/14428
Исследование эффектов взаимодействия в тесных двойных системах с нерелятивистскими компонентами / Академия наук Эстонии, Тартуская астрофизическая обсерватория имени В. Струве. – Таллинн : Валгус, 1990. – 90 с. : ил. – ISBN 5-440-01095-5 : 1. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: On the features of circumstellar shells in semi-separated close binary systems and modeling of their light curves.
21. Н/8977/Пр-2032
Источник SLX1732-304 в шаровом скоплении Терзан 1. Спектральные состояния и рентгеновский всплеск / М. Н. Павлинский, С. А. Гребенев, А. А. Лутовинов [и др.]. – Москва, 2000. – 19 с. : ил. – (Препринт / Институт космических исследований (Москва) ; Пр-2032). – Текст : непосредственный.
Abstract: This paper presents the results of observations of the X-ray barster SLX1732-304 in the Terzan 1 globular cluster by the ART-P telescope of the GARNET Observatory.
22. Н/11110/81-91
Каждан, Я. М. Выход ударной волны на поверхность звезды и последующее расширение вещества в вакуум – описание с учетом сферичности геометрии / Я. М. Каждан, М. В. Мурзина. – Москва, 1991. – 38 с. : ил. – (Препринт / Институт теоретической и экспериментальной физики (Москва) ; 81-91). – Текст : непосредственный.
Abstract: A solution to the problem of the shock wave exiting onto the surface of a star and the subsequent expansion of matter into a vacuum is constructed, taking into account the sphericity of geometry in the first order in the vicinity of the boundary of the star.
23. Ар20-2728
Калашников, И. Ю. Устойчивость течений в астрофизических объектах и лабораторных экспериментах : специальность 01.04.02 «Теоретическая физика» : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Калашников Илья Юрьевич ; Национальный исследовательский ядерный университет «МИФИ». – Москва, 2019. – 25 с. : ил. – Библиогр.: с. 23-25. – Текст : непосредственный.
24. Н/11110/12-12
Кошкарев, Д. Г. О вспышке сверхновой 1987А / Д. Г. Кошкарев. – Москва : ИТЭФ, 2012. – 5 с. : ил. – (Препринт / Институт теоретической и экспериментальной физики (Москва) ; 12-12). – Библиогр.: с. 5 (8 назв.). – Текст : непосредственный.
Abstract: It is assumed that a supernova light flash occurs at the beginning of a star's transition from an equilibrium state in which the pressure of gravity is balanced by the pressure of a degenerate electron gas to a new equilibrium state in which the pressure of gravity is balanced by the pressure of a degenerate neutron gas. This assumption rearranges the neutrino pulse and the supernova flash in time. The consequences of the obtained results are discussed.
25. М/16400/6 за 2019 г.
Легкоступов, М. С. К вопросу об астрофизических исследованиях протопланетных дисков звезд / М. С. Легкоступов. – Москва : ИПМ им. М. В. Келдыша РАН, 2019. – 20 с. – (Препринт / Институт прикладной математики имени М. В. Келдыша (Москва), ISSN 2071-2898 ; 6 за 2019 г.). – Библиогр.: с. 16-19 (40 назв.). – Текст : непосредственный.
Abstract: A brief analytical review of selected works on astrophysical observations of protoplanetary disks of stars is presented. It is shown that the data of astrophysical observations generally confirm the validity of the protoplanetary ring model – a model of the formation of planetary systems of stars, which is based on the origin and development of large-scale gravitational instabilities (protoplanetary rings) in the protoplanetary disk of stars.
26. Д10-15/27627
Липунов, В. М. Астрофизика нейтронных звезд / В. М. Липунов. – 2-е изд., доп., репринт. – Москва : Рус. Мiръ, 2015. – 302 с. : ил. – Библиогр.: с. 286-302. – ISBN 978-5-89577-196-9. – Текст : непосредственный.
Abstract: The problems of a new, rapidly developing field of modern astrophysics – the astrophysics of neutron stars are presented. The observed manifestations of neutron stars are described – radio pulsars, X-ray pulsars, transient X-ray sources, X-ray bursters, sources of gamma-ray bursts. The author concerns not only established views, but also problems (and there are many of them) that have yet to be solved. For physicists and astronomers-specialists, postgraduates and students.
27. Д9-09/55454
Липунов, В. М. В мире двойных звезд / В. М. Липунов. – 2-е изд. – Москва : URSS, 2009 (М.). – 253 с. : ил. – (Науку – всем! Шедевры научно-популярной литературы). – ISBN 978-5-397-00023-9. – Текст : непосредственный.
Abstract: It is popular to talk about new discoveries, ideas and hypotheses in the field of studying binary stars. The sequence of presentation corresponds to the successive stages of the life (evolution) of binary stars. But the story of each stage is based on the example of a specifically observed binary system with a description of the living history of its discovery and research. At the same time, the essence of the main astrophysical methods of studying binary systems is revealed.
28. Масленникова, Н. А. Симбиотическая природа циркониевой звезды CSS 1102 / Н. А. Масленникова, А. А. Татарникова, А. М. Татарников, Н. П. Иконникова, А. В. Додин. – Text : electronic // Письма в Астрономический журнал. – 2022. – №1. – С. 43-51. – ISSN: 0320-0108. – URL: https://elibrary.ru/item.asp?id=47988449 (дата обращения: 05.07.2022). – Access mode: Scientific Electronic Library eLIBRARY.RU.
Abstract: According to the results of spectral observations carried out on the 2.5-m telescope of the KGO GAISH, the symbiotic nature of the little-studied S-star CSS 1102 has been established. A Balmer jump in emission is observed in the spectrum of the object and there are lines characteristic of gas nebulae (HI, HeI and [NeIII]). The analysis of the energy distribution showed that, in addition to the nebula and the cold component of the spectral class S4.5/2, there is a noticeable excess radiation in the blue and near UV ranges in the CSS 1102 spectrum, which can be attributed to an accretion disk. Photometric monitoring performed on the 60-cm telescope of the KGO GAISH in band B revealed the presence of rapid variability on a time scale of tens of minutes and an amplitude of several percent, which is an additional argument in favor of the existence of an accretion disk in the system.
29. Ар19-2060
Моисеева, А. В. Фундаментальные параметры выборки СР звезд по результатам спектроскопии на 6-м телескопе : специальность 01.03.02 «Астрофизика и звездная астрономия» : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Моисеева А. В. ; Российская академия наук, Специальная астрофизическая обсерватория. – Посёлок Нижний Архыз (Карачаево-Черкесия), 2019. – 13 с. – Библиогр.: с. 12-13. – Текст : непосредственный.
30. Д1/31544
Мустель, Э. Р. Звездные атмосферы / Э. Р. Мустель ; редакционная коллегия: В. А. Амбарцумян [и др.]. – Москва : Гос. изд-во физ.-мат. литературы, 1960. – 444 с. : ил. ; 21 см. – (Проблемы теоретической астрофизики). – Библиогр.: с. 435-444 (204 назв.). – Текст : непосредственный.
Abstract: The issues related to the physical structure of stellar photospheres are considered and the analysis of absorption lines in the spectra of stars is given. Observations of the closest of them, the Sun, allowed us to establish that its atmosphere can be divided into a number of layers that differ from each other in their physical characteristics.
31. Ж2-90/14636
Нестационарные процессы в тесных двойных системах : материалы всесоюзного совещания, Тыравере, 10-14 октября 1989 г. / под редакцией И. Пустыльника. – Б. м. : [б. и.], 1990. – 113 с. : ил. – В надзаг.: АН Эстонии, Тарт. астрофиз. обсерватория им. В. Струве. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The collection contains the contents of 21 reports and reports made at the All-Union Meeting "Non-stationary processes in close binary systems" in the period from October 10 to October 14, 1989 in Tyraver. The reports are mainly devoted to new observational data and their interpretation of eclipsed binary systems with non-relativistic components, as well as some symbiotic stars.
32. Н/11110/5-99
Нечпай, В. И. Простая модель сжатия сверхновых / В. И. Нечпай, Л. Ф. Потапкина, С. А. Холин. – Москва, 1999. – 13 с. : ил. – (Препринт / Институт теоретической и экспериментальной физики (Москва) ; 5-99). – Текст : непосредственный.
Abstract: To study the effect of the equation of state, magnetic fields, neutrino yield, nucleosynthesis processes on a supernova explosion, a relatively simple gas-dynamic model of compression (and expansion) is proposed, which allows generalization to the relativistic case (motion with velocities close to the speed of light).
33. Н/13643/662
Обзор областей звездообразования, связанных с ИК-источниками, в линии J=1-0 молекулы СО и ее изотопов. Результаты наблюдений в линии С18О(J=1-0) / Н. Р. Троицкий [и др.]. – Нижний Новгород, 2004. – 15 с. : ил. – (Препринт / Институт прикладной физики (Нижний Новгород) ; 662). – Библиогр.: с. 15 (9 назв.). – Текст : непосредственный.
Abstract: The results of observations of 23 dense nuclei of molecular clouds associated with "cold" infrared sources IRAS in the line J=1-0 of the C18O molecule are presented. The observations were carried out on the 13.7-meter radio telescope of the Purple Mountain Observatory, China. The C18O line (J=1-0) is registered in the radiation of 21 objects. In the approximation of local thermodynamic equilibrium, the radiation concentrations of C18O and H2 molecules were estimated in the direction of the maximum of the integral intensity of C18O radiation, which were (2.5-10.4)·1015 cm-2 and (1.5-6.1)·1022 cm-2, respectively. Kinetic temperatures determined by CO lines for these maxima range from 14 to 45 K. For six objects for which the maps can be considered almost complete, the sizes of the C18O radiation regions ranging from 0.5 to 1.2 pc are estimated. The masses of these objects lie in the range (390-1750) Mo and are close to the estimates following from the virial theorem. The range of average densities of objects was (0.3-1.4)·104 cm-3.
34. Д7-91/98330
Орленок, В. В. Физика Земли, планет и звезд : учебное пособие / В. В. Орленок. -Калининград, 1991. – 174 с. : ил. – ISBN 5-230-08765-X. – В надзаг.: Калинингр. гос. ун-т. – Библиогр.: с. 171-173 (49 назв.). – Текст : непосредственный.
Abstract: The internal structure and physical state of matter in the bowels of the Earth, planets and stars are considered. The ideas about the unity of the chemical composition of proto-matter in all objects of the Solar system and the surrounding outer space are substantiated. The stellar and planetary paths of proto-matter evolution are considered. It is shown that these processes are based not so much on the differences in the chemical composition of the initial cosmic formations, as on the difference in their masses. New data on the structure and evolution of the Earth allow us to better understand the nature of other planets, the Sun and stars, which in turn have a huge impact on the life of our planet. Information about the planetary and stellar state of matter is considered primarily from the standpoint and from the point of view of terrestrial geographical and geological-geophysical problems.
35. М/14605/ITP-90-37E
Пилюгин, Л. С. On the chemical evolution of star formation regions in blue dwarf galaxies / Л. С. Пилюгин. – Kiev, 1990. – 24 p. : il. – (Препринт / Институт теоретической физики (Киев) ; ITP-90-37E). – Перед загл. авт.: L. S. Pilyugin. – Bibliogr.: p. 13-15. – Текст : непосредственный.
Abstract: The evolutionary changes in the oxygen content in gas in the star formation regions of HII galaxies are considered. It is shown that the oxygen content in the gas in the star formation regions changes significantly during evolution. The calculated evolutionary tracks of the star formation regions of HII galaxies in the O/H-WHß and WHß-NLc diagrams are in agreement with the observed positions of HII galaxies in these diagrams.
36. М/14605/ITP-90-73E
Пилюгин, Л. С. On the gaseous oxygen abundance evolution of star formation regions of hii galaxies / Л. С. Пилюгин. – Kiev, 1990. – 20 p. : il. – (Препринт / Институт теоретической физики (Киев) ; ITP-90-73E). – Перед загл. авт.: L. S. Pilyugin. – Библиогр.: с. 12-14. – Текст : непосредственный.
Abstract: Evolutionary changes in the oxygen content in gas in the regions of star formation of NI galaxies are considered. It is shown that the oxygen content in the gas in the star formation regions changes significantly during their evolution.
37. R/5815/AE-98/10
Ряжская, О. Г. Presupernova y-burst and some consequences of vep-reaction / О. Г. Ряжская. – S.l. : [s. n.], 1998. – 7 p. – ([Pubblicazione] INFN / Ist. naz. di fisica nucleare ; AE-98/10). – Библиогр.: с.7. – Текст : непосредственный.
Abstract: The production of g-burst by absorption of neutrino emission of a collapsing star in its envelope consisting of either hydrogen or carbon; the possible detection of soundless collapse using neutrino and g-ray telescopes, the possible explosion of the hydrogen-containing objects near the collapsing stars, and other consequences of nA e interaction with the protons in the star are discussed. PACS 97.30.Qt – Novae, dwarf novae, recurrent novae, and other cataclysmic (eruptive) variables.
38. J2/26649
Саакян, Г. С. Физика нейтронных звезд / Г. С. Саакян. – 2 изд., перераб., доп. – Ереван : Изд-во Ерев. гос. ун-та, 1998. – 306 с. : ил. – Библиогр.: с. 294-297. – Указ.: с. 300-303. – Текст : непосредственный.
Abstract: The monograph is devoted to a systematic presentation of the theory of neutron stars, pulsars and bursters. The first part contains a detailed exposition of the theory of degenerate stellar matter for the entire range of densities. The second part is devoted to stellar configurations of such matter (white dwarfs and neutron stars). Due attention is also paid to the manifestations of neutron stars, such as pulsars and point sources of X-ray radiation: two extensive chapters are devoted to them. Chapter VI provides a brief and accessible exposition of the basics of the relativistic theory of gravity, knowledge of which is necessary for mastering the material of the following chapters.
39. М/55364/1
Сахибуллин, Н. А. Методы моделирования в астрофизике / Н. А. Сахибуллин. – Казань : Фэн, 19 – . – В надзаг.: АН Татарстана. Отд-ние физики, энергетики и наук о Земле. – Текст : непосредственный.
1 : Звездные атмосферы. – 1997. – 328 с. : ил. – Библиогр.: с. 317-328.
Abstract: The monograph is devoted to the presentation of the achievements of the last decade in the field of implementation of modern numerical modeling methods in astrophysics. Special emphasis is placed on the issue of constructing models of stellar atmospheres and obtaining their theoretical radiation spectra. At the same time, not only a description of the methods is given, but also specific recommendations for their application are given, based on the author's many years of scientific experience. As concrete examples illustrating the progress in the field of modeling, some results obtained in recent years by the Kazan group of astrophysicists are given. The book is intended for students, postgraduates and specialists dealing with the problems of radiation transfer and the formation of star spectra.
40. Ар18-6613
Сендзикас, Е. Г. Спектроскопическое исследование далеко проэволюционировавших звезд : специальность 01.03.02 : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Сендзикас Е. Г. ; Специальная астрофизическая обсерватория Российской академии наук. – пос. Нижний Архыз (Карачаево-Черкесия), 2018. – 15 с. – Библиогр.: с. 14-15 (13 назв.). – Текст : непосредственный.
41. Д10-21/88133
Соколов, Д. Небесные магниты : природа и принципы космического магнетизма / Дмитрий Соколов. – Москва : Альпина нон-фикшн, 2021. – 158, [1] с. – Библиогр.: с. 149-153. – ISBN 978-5-00139-336-8. – Текст : непосредственный.
Abstract: Dmitry Sokolov's book is conceived not as a study of the world of physical phenomena, but in many ways as a saga about science itself. Talking about magnetic fields, the author seeks to show how and for what physicists work. How are the magnetic fields of distant stars arranged? Where do they come from, how do they differ, how and what do they affect? How can the Earth's magnetic field be changed and what are the ways to observe it? What is the phenomenon of the Kursk magnetic anomaly? What is the structure of the magnetic fields of spiral galaxies and the Sun and how are the magnetic cycles associated with them, which scientists have been trying to track since ancient times? The answers to these and many other questions are accompanied by entertaining stories from the life of scientists and the history of domestic and world science.
42. Д9-06/23254
Тесные двойные звезды в современной астрофизике : тезисы докладов Всероссийской астрономической конференции, 22-24 мая 2006 г. : к 100-летию со дня рождения Д. Я. Мартынова / редактор К. А. Постнов. – Москва : [б. и.], 2006 (М.). – 56 с. : ил. – Авт. указ.: с. 53-54. – ISBN 5-9900318-3-1. – В надзаг.: МГУ им. М. В. Ломоносова, Гос. астрон. ин-т им. П. К. Штернберга. – Часть текста англ. – Текст : непосредственный.
Abstract: Binary stars are natural laboratories in which the study of the motion and interaction of components allows us to find the most important stellar characteristics: masses, sizes, temperatures, internal structure. Therefore, double stars have always been given great attention in astrophysical research. Binary stars with compact relativistic components are by far one of the most accurate tools for testing the theory of the structure and evolution of both ordinary and degenerate remnants and black holes. The unique properties and features of TDS with compact relativistic objects are determined primarily by the processes of accretion of matter from a normal star to a compact component. The huge gravitational energy released during accretion to compact stars is processed into heat and radiated in a hard electromagnetic range. The physics of such processes was first understood and developed in our country in the mid-60s – early 70s of the XX century in the pioneering works of Ya. B. Zeldovich, I. S. Shklovsky and their students. Long-term optical observations of eclipsed TDS in non-circular orbits, conducted by D. Y. Martynov and his students, provided a unique opportunity to study the movement of the apse line and thereby investigate the internal structure of stars and verify fundamental theories of gravity.
43. М/14715/1558
Урпин, В. А. Magnetic field decay in netron star crust / В. А. Урпин, А. Г. Муслимов. – Leningrad, 1991. – 25 p. – (Препринт / Физико-техн. ин-т им. А. Ф. Иоффе (Ленинград) ; 1558). – Перед загл. авт.: V. A. Urpin, A. G. Muslimov. – Текст : непосредственный.
Abstract: The evolution of the magnetic fields of neutron stars, initially concentrated in relatively shallow layers of their shells with a density of p ≤, is considered po = 4 ⁎ 1011 g/cm3. The effect of the cooling of the star on the conductivity of matter and on the rate of field dissipation is taken into account.
44. Урысон, А. В. О звездах : научно-популярное издание / А. В. Урысон. – Долгопрудный : Издательский Дом «Интеллект», 2018. – 120 c. – ISBN 978-5-91559-227-7. – URL: https://www.iprbookshop.ru/103493.html (дата обращения: 05.07.2022). – Access mode: for authorized users. – Text : electronic.
Abstract: The return of astronomy to the curriculum of Russian schools after a break of more than twenty years requires the appearance of modern textbooks, especially introductory books. A compact manual about the most important objects of the surrounding world was created by an active astrophysicist. In it, the reader will find an amazing fusion of popular science and educational material reflecting the most important achievements of the XX and XXI centuries. The development of physics and technology made it possible to make cardinal discoveries in observational astronomy, which changed ideas about the Universe and gave a powerful impetus to physics itself. The book is written in excellent language, clearly and intelligibly, at the level of the best examples of Russian popular science literature. For an audience from schoolchildren to students and adults engaged in self-education.
45. Ж2-20/70001
Физика звезд средних и малых масс с активностью солнечного типа : [монография] / Р. Е. Гершберг, Н. И. Клиорин, Л. А. Пустильник, А. А. Шляпников. – Москва : ФИЗМАТЛИТ, 2020. – 767 с. : ил. – Библиогр.: с. 662-751, 766-767. – Пред. указ.: с. 752-758. – ISBN 978-5-9221-1881-1. – Текст : непосредственный.
Abstract: The monograph systematizes and summarizes the results of studies of solar-type activity inherent in a significant part of the stars of medium and small masses of the Galaxy, describes the characteristics of such stars in a calm state, during sporadic outbursts and changes in such activity over evolutionary times. The data of observations obtained in the entire range of the electromagnetic spectrum from decameter radio waves to X-rays are described in detail. In two theoretical chapters, modern models of flares and models of stellar dynamos are considered. The appendix describes a catalog of stars with solar-type activity. The book is intended for researchers engaged in the study of the physics of stars and the Sun, graduate students and students of astrophysical specialties and specializing in the field of ground and space research.
46. Н/8183/ INP 96-3
Хриплович, И. Б. Gravitational interaction of spinning bodies, center-of-mass coordinate and radiation of compact binary systems / И. Б. Хриплович, А. А. Померанский. – Novosibirsk, 1996. – 15 p. – (Препринт / Институт ядерной физики им. Г. И. Будкера (Новосибирск) ; INP 96-3). – Текст : непосредственный.
Abstract: Spin-orbit and spin-spin effects in the gravitational interaction are treated in a close analogy with the fine and hyperfine interactions in atoms. The proper definition of the cener-of-mass coordinate is discussed. The technique developed is applied then to the gravitational radiation of compact binary stars. Our result for the spin-orbit correction differs from that obtained by other authors. New effects possible for the motion of a spinning particle in a gravitational field are pointed out. The corresponding corrections, nonlinear in spin, are in principle of the same order of magnitude as the ordinary spinspin interaction
47. М/38461/38
Чернин, А. Д. Звезды и физика / А. Д. Чернин. – 2-е изд., испр. и доп. – Москва : Наука. Физматлит, 2004. – 174 с. : ил. – («Квант». Библиотечка ; Вып. 38). – ISBN 5-354-00559-0. – Текст : непосредственный.
Abstract: Pulsars, flashing X–ray stars, the amazing star SS 433, the corona of galaxies, quasars, relic radiation are the main topics of the book. It tells about the physical processes that determine the observed astronomical phenomena, about the latest hypotheses and models, about the mysteries of astrophysics that have yet to be solved. The book is intended for high school students, students, teachers.
48. Д9-09/59316
Шварцшильд, М. Строение и эволюция звезд / М. Шварцшильд ; перевод с английского Э. В. Кононовича ; под редакцией с предисловием А. Г. Масевич. – 4-е изд. – Москва : URSS, 2009 (М.). – 436 с. : ил. – (Физико-математическое наследие: физика (астрономия)). – Библиогр.: с. 420-432. – Предм. указ.: с. 433-436. – ISBN 978-5-397-00759-7. – Текст : непосредственный.
Abstract: The book by the famous American astronomer M. Schwarzschild is devoted to one of the most interesting problems of modern astrophysics – the internal structure and evolution of stars. It consistently, with great pedagogical skill, outlines the basics of the theory of the internal structure of stars, the principles of calculating stellar models and comparing the theory with observations. The final chapter of the book gives a picture of stellar evolution according to modern concepts. The book will be read with great interest by astronomers – both specialists and students. But it will be of interest to physicists, mathematicians, and geophysicists who wish to familiarize themselves with the physical problems put forward by the theory of stellar structure, as well as with the mathematical methods used by modern astrophysics. The simplicity and clarity of the presentation make most of the book, especially the chapters on stellar evolution, accessible to non-specialists.
49. Юдин, А. В. Взрыв нейтронной звезды минимальной массы в рамках релятивистской гидродинамики / А. В. Юдин. – Text : electronic // Письма в Астрономический журнал. – 2022. – №6. – С. 393-402. – ISSN:0320-0108. – URL: https://elibrary.ru/item.asp?id=48659249 (дата обращения: 05.07.2022). – Access mode: Scientific Electronic Library eLIBRARY.RU.
Abstract: The equations of relativistic hydrodynamics are adapted for the spherically symmetric case and the Lagrangian form of the notation. With their help, the process of explosive destruction of a neutron star of minimal mass – the key ingredient of the model of stripping short gamma-ray bursts - is modeled. The process of the shock wave exiting onto the surface of a neutron star, accompanied by the acceleration of matter to ultrarelativistic velocities, has been studied. A comparison with the results of previously published non-relativistic calculations is carried out.
50. Astrophysics and space science : from X-Ray binaries to quasars: black holes on all mass scales / editor : T. J. Maccarone [et al.]. – Electronic text data. – Dordrecht : Springer, 2005. – 288 p. – ISBN 978-1-402-04085-6. – URL: http://dx.doi.org/10.1007/1-4020-4085-7 (дата обращения: 28.06.2022). – Access mode: for authorized users.
Abstract: This volume brings together contributions from many of the world's leading authorities on black hole accretion. The papers within represent part of a new movement to make use of the relative advantages of studying stellar mass and supermassive black holes and to bring together the knowledge gained from the two approaches. The topics discussed here run the gamut of the state of the art in black hole observational and theoretical work-variability, spectroscopy, disk-jet connections, and multi-wavelength campaigns on black holes are all covered.
51. Н/11110/43-93
Benvenuto, O. G. Possible signatures of the conversion of a neutron star to a strange star / O. G. Benvenuto, M. I. Krivoruchenko, B. V. Martemyanov. – Moscow, 1993. – 24 p. – (Препринт / Институт теоретической и экспериментальной физики (Москва) ; 43-93). – Библиогр.: с. 20-24 (55 назв.). – Текст : непосредственный.
Abstract: The problem of the identification of strange stars is discussed. We suggest some characteristic signatures for the search for strange stars: a two-step mechanism for supernova explosions accompanied by the occurrence of strange stars and two neutrino bursts; microstructure analysis in the profile of pulsar emission; and unusual stability in the rotation of millisecond pulsars due to the absence of internal crust in strange stars. The cooling of strange stars is faster than the cooling of ordinary neutron stars, so low surface temperature of pulsars can indicate the existence of massive quark cores in observed pulsars. Low mass strange stars as bursters and/or X-ray sources have peculiar observable features: low luminosity and (for bursters) high recurrence rate, large duration of bursts, low ratio of energy emitted between two bursts and energy emitted during the burst.
52. Camenzind, M. Compact objects in astrophysics : white dwarfs, neutron stars and black holes / M. Camenzind. – Electronic text data. – Berlin ; Heidelberg : Springer, 2007. – 682 p. – (Astronomy and astrophysics library, ISSN 0941-7834). – ISBN 978-3-540-49912-1. – URL: http://dx.doi.org/10.1007/978-3-540-49912-1 (дата обращения: 28.06.2022). – Access mode: for authorized users.
Abstract: Modern comprehensive introduction and overview of the physics of White Dwarfs, Neutron Stars and Black Holes, including all relevant observations. Contains a basic introduction to General Relativity, including the modern 3+1 split of spacetime and of Einstein’s equations. The split is used for the first time to derive the structure equations for rapidly rotating neutron stars and Black Holes. Detailed discussions and derivations of current theoretical results. In particular also the most recent equations of state for neutron star matter are explained. Topics , such as colour superconductivity are discussed and used for modelling. A book for graduate students and researchers containing exercises and solutions.
53. Close binaries in the 21st century: new opportunities and challenges / editor Г. Gimenez [et al.]. – Electronic text data. – Dordrecht : Springer, 2006. – 401 p. – ISBN 978-1-4020-5027-5. – URL: http://dx.doi.org/10.1007/978-1-4020-5027-5 (дата обращения: 28.06.2022). – Access mode: for authorized users.
Abstract: Contributions to this conference covered the latest achievements in the field and reflected the state of the art of the dynamically evolving area of binary research.
54. Cosmic explosions : on the 10th anniversary of SN1993J (IAU colloquium 192) / editors J. Marcaide, K. W. Weiler. – Electronic text data. – Berlin ; Heidelberg : Springer, 2005. – 592 p. – (Springer proceedings in physics, ISSN 0930-8989 ; 99). – ISBN 978-3-540-26633-4. – URL: http://dx.doi.org/10.1007/b137830 (дата обращения: 28.06.2022). – Access mode: for authorized users.
The proceedings of the conference Supernovae 2003 (IAU colloquium 192) provides an extensive state-of-the-art survey of all theoretical and observational aspects of supernovae and gamma-ray bursts, as well as their impact on cosmology. This volume offers everyone working in this field an authoritative and comprehensive source of reference.
55. Kogure, T. The astrophysics of emission-line stars / T. Kogure, K. Leung. – Electronic text data. – New York, NY : Springer-Verlag, 2007. – 537 p. – (Astrophysics and space science library, ISSN 0067-0057 ; 342). – ISBN 978-0-387-68995-1. – URL: http://dx.doi.org/10.1007/978-0-387-68995-1 (дата обращения: 28.06.2022). – Access mode: for authorized users.
Abstract: Many types of stars show conspicuous emission lines in their optical spectra. These stars are broadly referred to as emission line stars. Emission line stars are attractive to many people because of their spectacular phenomena and their variability. The Astrophysics of Emission Line Stars offers general information on emission line stars, starting from a brief introduction to stellar astrophysics, and then moving toward a broad overview of emission line stars including early and late type stars as well as pre-main sequence stars. Detailed references have been prepared along with an index for further reading.
56. Maeder, A. Physics, formation and evolution of rotating stars / A. Maeder. – Berlin ; Heidelberg : Springer, 2009. – 829 p. – (Astronomy and astrophysics library, ISSN 0941-7834). – ISBN 978-3-540-76949-1. – URL: http://dx.doi.org/10.1007/978-3-540-76949-1 (дата обращения: 28.06.2022). – Access mode: for authorized users.
Abstract: Rotation is ubiquitous at each step of stellar evolution, from star formation to the final stages, and it affects the course of evolution, the timescales and nucleosynthesis. Stellar rotation is also an essential prerequisite for the occurrence of Gamma-Ray Bursts. In this book the author thoroughly examines the basic mechanical and thermal effects of rotation, their influence on mass loss by stellar winds, the effects of differential rotation and its associated instabilities, the relation with magnetic fields and the evolution of the internal and surface rotation. Further, he discusses the numerous observational signatures of rotational effects obtained from spectroscopy and interferometric observations, as well as from chemical abundance determinations, helioseismology and asteroseismology, etc. On an introductory level, this book presents in a didactical way the basic concepts of stellar structure and evolution in «track 1» chapters. The other more specialized chapters form an advanced course on the graduate level and will further serve as a valuable reference work for professional astrophysicists.
57. R/6714/162
Physical processes in fragmentation and star formation : proceedings of the workshop on physical processes in fragmentation and star formation, Held in Monteporzio Catone (Rome), Italy, June 5-11, 1989 / editor R. Capuzzo-Dolcetta. – Dordrecht [etc.] : Kluwer, 1990. – 469 p. : ill. – (Astrophysics and space science library / ed.: J. E. Blamont ; vol.162). – ISBN 0-7923-0769-0. – Библиогр.в конце ст. – Текст : непосредственный.
Abstract: Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner.
58. R/7069/369
Physics of classical novae : proceedings of colloquium N 122 of the International astronomical union, Madrid, 27-30 June 1989 / International astronomical union ; ed. A. Cassatella ; ed. R. Viotti. – Berlin : Springer, 1990. – 12, 462 p. : ill. – (Lecture notes in physics, ISSN 0075-8450 ; N 369). – ISBN 3-540-53500-4. – Указ.: с. 455-462. – Текст : непосредственный.
Abstract: Satellite observations in various previously unexplored spectral regions have provided a host of data on novae over the last decade. This carefully refereed conference volume is devoted to classical novae and related objects. Around 30 papers discuss observations (basic properties of novae, outbursts, and nebular ejecta), theoretical considerations, and models of observations. In addition the reader will find an introductory review on binary stars by R.P. Kraft and a summary by P. Eggleton of the papers and posters presented at the conference. To help the reader in finding any specific subject or stellar object the volume concludes with a detailed index.
59. R/6714/157
Physics of luminous blue variables : proceedings of the 113-th colloquium of the intern. astronomical union, held at Val Morin, August 15-18, 1988 / editor K. Davidson. – Dordrecht : Kluwer acad. publ, 1989. – 315 p.: ill. – (Astrophysics and space science library / ed.: J. E. Blamont ; Vol.157). – ISBN 0-7923-0443-8. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: A strange field of speculation is opened by this phenomenon here we have a star fitfully variable to an astonishing extent and whose fluctuations are spread over centuries. Apparently in no settled period and with no regularity of progression. What origin can we ascribe to these sudden flashes and relapses? What conclusions are we to draw as to the comfort or habitability of a system depending for its supply of light and heat on so uncertain a source? J. F. W. Herschel! We can imagine, at least, that the study of Luminous Blue Variable stars began as the official court astrophysicists of Eridu speculated about a new 5000 years ago first-magnitude star which persisted in their southern sky for several years. After that the topic languished for a while, but now it has been renewed following recent observations by Blaeu (P Cygni, c.1600) and Herschel (1 Argus, c.1840). More soberly, it is only within the past few years that we have begun to understand LBV's and to recognize their coherence as a class. Thus, only a minority of astronomers are familiar yet with this relatively new topic, whose potential implications are of great interest (see below). One purpose of this book, we hope, will be to provide an accessible overview of the subject for interested astronomers and astrophysicists in general.
2. Heliophysics (physics of the Sun)
60. Авакян, С. В. Физика солнечно-земных связей : некоторые результаты, проблемы и новые подходы / С. В. Авакян. – Text : electronic // Геомагнетизм и аэрономия. – 2008. – №4. – С. 435-442. – ISSN: 0016-7940. – URL: https://elibrary.ru/item.asp?id=11532815 (дата обращения: 05.07.2022). – Access mode: Scientific Electronic Library eLIBRARY.RU
Abstract: The results of the work carried out in the field of the most pressing problems of physics and optics of solar-terrestrial connections are analyzed. This is a problem of energy in the physics of the ionosphere, considered in connection with the problem of the absence to date of constant space monitoring, ionizing the upper atmosphere of the solar radiation flux. These are the problems of converting the energy of solar flares and corpuscular eruptions into microwave ionospheric radiation. And finally, this is the main problem of modern natural science – the physical mechanism of solar-terrestrial connections in the application to the explanation of the detected correlations in the systems "Sun – weather" and "Sun – biosphere". A single physical (radio-optical) mechanism for controlling processes in the lower atmosphere and the biosphere (including humans) is considered, due to the magnitude of the level of solar and geomagnetic activity associated with ionospheric microwave radiation in transitions between optically highly excited (Rydberg) states of all upper atmospheric components.
61. М/60208/1
Актуальные проблемы физики солнечной и звездной активности : конференция стран СНГ и Прибалтики, Нижний Новгород, 2-7 июня 2003 г. : сборник докладов в 2-х томах / Институт прикладной физики. – Нижний Новгород, 20 – . – Текст : непосредственный.
Т. 1. – 2003. – С. 3-266 : ил. – ISBN 5-8048-0041-8. – Библиогр. в конце ст.
Abstract: This collection contains reports of the Conference of the CIS and Baltic countries "Actual problems of physics of solar and stellar activity", held on June 2-7, 2003 at the Scientific Research Radiophysical Institute (NIRFI) Ministry of Education of the Russian Federation (Nizhny Novgorod). The works present the latest theoretical and experimental results on the physics of solar activity phenomena and processes in the solar wind and heliosphere, on solar-stellar analogies, on the mechanisms of radiation and wave propagation in the magnetospheres of stars and planets, on the influence of solar activity on near-Earth space and terrestrial processes. The collection is of interest to specialists in these areas, as well as to students and postgraduates in the specialties "Astrophysics and radio astronomy", "Radiophysics", "Instruments and methods of experimental physics", "Heliophysics and physics of the Solar system".
62. М/60208/2
Актуальные проблемы физики солнечной и звездной активности : конференция стран СНГ и Прибалтики, Нижний Новгород, 2-7 июня 2003 г. : сборник докладов в 2-х томах / Институт прикладной физики. – Нижний Новгород, 20 – . – Текст : непосредственный.
Т. 2. – 2003. – С. 271-530 : ил. – ISBN 5-8048-0044-2. – Библиогр. в конце ст. – Именной указ.: с. 527-530
Abstract: This collection contains reports of the Conference of the CIS and Baltic countries "Actual problems of physics of solar and stellar activity", held on June 2-7, 2003 at the Scientific Research Radiophysical Institute (NIRFI) Ministry of Education of the Russian Federation (Nizhny Novgorod). The works present the latest theoretical and experimental results on the physics of solar activity phenomena and processes in the solar wind and heliosphere, on solar-stellar analogies, on the mechanisms of radiation and wave propagation in the magnetospheres of stars and planets, on the influence of solar activity on near-Earth space and terrestrial processes. The collection is of interest to specialists in these areas, as well as to students and postgraduates in the specialties "Astrophysics and radio astronomy", "Radiophysics", "Instruments and methods of experimental physics", "Heliophysics and physics of the Solar system".
63. Д10-14/17872
Алтынцев, А. Т. Введение в радиоастрономию Солнца / А. Т. Алтынцев, Л. К. Кашапова ; Иркутский государственный университет. – Иркутск : ИГУ, 2014. – 203 с. : ил. – (Солнечно-земная физика). – Библиогр.: с. 180-203. – ISBN 978-5-9624-1055-5. – Текст : непосредственный.
Abstract: It is part of the interdisciplinary course "Solar-Terrestrial Physics", taught at the Institute of Solar-Terrestrial Physics SB RAS (ISSF) to graduate students and undergraduates of the ISSF and Irkutsk State University. The main mechanisms of solar plasma radiation are consistently described, on the basis of which explanations of the nature of many solar objects are given. Introduces readers to modern achievements in the physics of the solar atmosphere, demonstrates the effectiveness of combining the radio astronomy method and methods using spacecraft (X-ray and ultraviolet ranges). It is also intended to support the course "Physics of the Sun", studied at the Physics Faculty of the University by students of the direction 011200 62 "Physics". Useful for undergraduate and graduate students specializing in astrophysics.
64. Д10-13/11693
Аннушкин, Ю. В. Введение в астрономию. Физика Солнечной системы : учебное пособие / Ю. В. Аннушкин, С. А. Язев. – Иркутск : Изд-во ИГУ, 2013. – 104 с. : ил. – (Солнечно-земная физика). – Библиогр.: с. 103 (15 назв.). – ISBN 978-5-9624-0886-6. – Текст : непосредственный.
Abstract: The manual gives the basic concepts and topics of the course of general astronomy in the application to the Solar System. Each section is provided with practical tasks and examples of their solutions. Successively, brief information from general astronomy, elements of celestial mechanics, the physical nature of planets and small bodies of the Solar system, elements of solar physics, questions of the origin and evolution of the Solar System are considered. The manual is intended for students of the Faculty of Physics.
65. Р2125
Астрономический вестник. Исследования солнечной системы / Российская академия наук, Институт прикладной математики имени М. В. Келдыша (Москва). – Москва : ИКЦ «Академкнига», 1967 – . – Перевод заглавия: Astronomical Herald (Table of Contents and Summaries in English). – Период.: 1967-1992 гг. – ежеквартально. – Журн. изд. МАИК «Наука/Интерпериодика» на англ. яз. – Журн. изд. под рук. Отд-ния физических наук РАН. – До 2019 г. изд-во: Наука. – Выходит раз в два месяца. – ISSN 0320-930X. – Текст : непосредственный.
Abstract: The journal publishes articles on the results of space and ground-based astronomical observations and theoretical studies of Solar system bodies, including their physical nature, motion, internal structure, chemical composition and properties of the atmosphere and surface, origin, evolution and dynamics. The journal "Astronomical Bulletin" also contains works on comparative planetology, cosmochemistry and cosmogony, reviews on the subject of the journal, articles on some theoretical issues related to the development of models, methods and measurement techniques. Short reports are also published, including information about scientific conferences, reviews of monographs, personalities.
66. Н/1181/215
Астрофизика и физика Солнца / редакционная коллегия: В. К. Абалакин (ответственный редактор) [и др.]. – Санкт-Петербург : [б. и.], 2000. – 375 с. : ил. – (Известия / Главная астрономическая обсерватория, ISSN 03677966 ; № 215). – В надзаг.: Рос. АН. – Библиогр. в конце ст. – Текст : непосредственный.
67. М/67482/2
Введение в физику Солнца : учебное пособие : в 2-х частях / Иркутский государственный университет, Институт солнечно-земной физики. – Иркутск : Изд-во ИГУ, 20 – . – Текст : непосредственный.
Ч. 2 / Р. Т. Сотникова [и др.]. – 2012. – 195 с. – Библиогр.: с. 193-195. – ISBN 978-5-9624-0622-0.
Abstract: The fundamentals of the theory of the formation of spectral lines and optical radiation of the Sun are discussed; the importance of radiation analysis in obtaining physical information about astrophysical objects is emphasized. On the basis of the "Electronic Atlas of the Solar Spectrum of the ISSF SB RAS", a computer workshop aimed at demonstrating spectral analysis methods and providing a research orientation of the educational process has been developed and presented. The basic concepts of modern physics of the solar corona, including the large-scale structure of the corona and coronal mass ejections, are presented. The problems of corona heating and its cyclicity are touched upon. The manual is intended for students and postgraduates specializing in astrophysics and solar physics.
68. Д8-93/12341
Глобальные вариации Солнца и физика активных областей : сборник научных трудов / Российская академия наук, Дальневосточное отделение, Уссурийская астрофизическая обсерватория ; редакционная коллегия: А. В. Баранов, Г. И. Корниенко, В. Ф. Чистяков (ответственный редактор). – Владивосток : Дальнаука, 1993. – 159 c. : ил. – ISBN 5-7442-0443-1. – Библиогр.в конце ст. – Текст : непосредственный.
Abstract: Global variations of the Sun are investigated: changes in the radius of the Sun with time and in connection with flares, differential rotation, meridional circulation of matter, periodic changes in flares and interplanetary magnetic fields, solar proton events and geomagnetic storms. The connection of flares with magnetic fields, the stratification of the physical parameters of the solar atmosphere in a magnetic field, and the influence of anomalous dispersion on the polarization parameters of spectral lines are considered. The results of observations of the Sun in the decameter range are presented.
69. М/42146/105
Голубчина, О. А. Квазисинхронная компонента динамики см-радиоизлучения локальных источников на Солнце / О. А. Голубчина. – Санкт-Петербург : [б. и.], 1994. – 13 c. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 105). – Текст : непосредственный.
Abstract: According to observations on RATAN-600 by the "relay" method J7, 29.07.81, a large–scale component – a quasi-synchronous component - of the radio emission dynamics of local sources identified on the photosphere of the Sun with groups of spots distant from each other at considerable distances was detected at 2.3 cm and 4.5 cm waves.
70. М/42146/124
Голубчина, О. А. О симпатических вспышках и всплесках, синхронных уярчениях локальных источников солнечного радиоизлучения и взаимодействии активных областей на Солнце в рентгеновском диапазоне / О. А. Голубчина. – Санкт-Петербург : [б. и.], 1997. – 49 с. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 124). – Текст : непосредственный.
Abstract: A review of studies of sympathetic flashes and bursts, synchronous brightening of local sources of solar radio emission, as well as interactions of active regions on the Sun according to X-ray observations is given.
71. М/42146/75 Спб
Голубчина, О. А. О синхронных повышениях относительных потоков локальных источников радиоизлучения Солнца и изменениях структур групп пятен за одни сутки по результатам наблюдений на λ = 2,3 см 9.10.02.80 г. на РАТАН-600 методом «эстафеты» / О. А. Голубчина. – Санкт-Петербург : [б. и.], 1992. – 41 с. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 75 Спб). – Текст : непосредственный.
Abstract: The work is devoted to the detection of synchronous brightenings of local sources (L. I.) at λ = 2.3 cm according to observations on RATAN-600 by the "relay" method. The methodology and accuracy of processing observations are discussed in detail. The reality of the existence of synchronous L. I. brightenings identified with groups of spots belonging not only to one complex with distances between spots up to ∆1 = 200o of heliographic longitude, but groups of spots spaced across the entire disk of the Sun with corresponding distances up to ∆1 = 80o is shown. During synchronous brightenings L. I. Solar services have registered either bursts of type 20, 21, 25, or (and) Ha-flares.Synchronous brightening of L. I. was detected during zalimbov Ha-flashes.The lower bound of the velocity of a possible disturbing agent is estimated: v > (2 – 2.5) ⁎ 103 km/s. The fact of detecting simultaneous (per day) changes in the structure of almost all groups of spots on the visible disk of the Sun and a change in the polarized radio emission of the corresponding local sources is given.
72. М/42146/120
Голубчина, О. А. Синхронные уярчения локальных источников СМ-радиоизлучения Солнца по наблюдениям на РАТАН-600 / О. А. Голубчина. – Санкт-Петербург : [б. и.], 1996. – 20 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Санкт-Петербург) ; 120). – Текст : непосредственный.
Abstract: The results of observations of local sources (L. I.) of solar radio emission in February 1980 and July 1981 at 2.3 cm and 4.5 cm waves on RATAN-600 are presented. The reality of the existence of synchronous brightenings of local sources spatially spaced apart relative to each other over considerable distances up to L>105 km is shown. Synchronous brightening of local sources was recorded at the moments of Ha-flashes and/or cm-bursts of various types: 3s, 5s, 8s, 28PRF, 31ABS, 45s, 20GRF, 21GRF, 30PBI.As a rule, synchronous brightenings of L. I. they are observed during an increase in solar radiation in soft X-rays. The lower bound of the velocity of the disturbing agent is (2-12) ⁎ 103 km/s. Frequent manifestations of synchronous brightenings of local sources in comparison with sympathetic bursts published by other authors allow us to refute the opinion about the exoticism of these phenomena.
73. Д8-92/912
Данные по солнечно-земной физике в машиночитаемой форме : материалы Мирового центра данных Б : Каталог. – Москва, 1992. -59 с. – Парал. загл. англ. – Текст рус., англ. – Текст : непосредственный.
Abstract: The catalog contains a description of that part of the archives of the World Data center B for solar-terrestrial physics (IDC for NWF), which has been translated into machine-readable form. Descriptions are given separately for each base or series of observations.
74. Д10-18/54835
Еселевич, В. Г. Ударные волны, возбуждаемые корональными выбросами массы / В. Г. Еселевич, М. В. Еселевич, И. В. Зимовец. – Москва : ФИЗМАТЛИТ, 2018. – 117 с. : ил. – Библиогр.: с. 112-117 (91 назв.). – ISBN 978-5-9221-1771-5. – Текст : непосредственный.
Abstract: The purpose of this monograph is to summarize the preliminary results of studies on the registration of shock waves in the Sun associated with coronal mass ejections. The most important physical results, which were predicted theoretically earlier, but have not yet been studied experimentally, include the observation of the phenomenon of "transition through the speed of sound" in a magnetized plasma with the formation of a collisional shock front, which has so far been observed only in gas, as well as the spatial resolution of the shock front profile with a characteristic width of the order of length the free path of protons. The third, most interesting and promising result, which has not yet been predicted theoretically, is the detection and experimental study of the transition from a collisional to a collisionless shock front. For researchers, postgraduates and undergraduates specializing in solar physics, astrophysics and plasma physics. The images shown on the cover were obtained using observations of coronal mass ejections on December 2, 2002 (front cover) and February 27, 2000. (back cover) with the LASCO instrument on board the SOHO spacecraft (a joint ESA/NASA project). The insert image on the front cover was obtained from observations of the coronal mass ejection on November 22, 2001 on the Mark-IV coronograph of the Mauna Loa Solar Observatory.
75. Н/8515/112
Исследования по геомагнетизму, аэрономии и физике Солнца : сборник научных трудов / Российская академия наук, Сибирское отделение, Институт солнечно-земной физики. – Новосибирск : Наука, 20 – . – Текст : непосредственный.
Вып. 112. – 2001. – 289 с. – Библиогр. в конце ст.
Abstract: The collection "Research on Geomagnetism, Aeronomy and Solar Physics", issue 112, presents the results of theoretical and experimental research on the main disciplines of solar-terrestrial physics. The first results of goniometric measurements of the wave field of Pc1-type geomagnetic pulsations performed at two mid-latitude observatories are reported. The features of the wind regime are described and estimates of general patterns and regional differences of the wind field are given in order to determine the climatic norms for the lower thermosphere. The ionospheric effects observed by various methods during magnetic storms are analyzed. The results of photometric observations at high-latitude and medium-latitude stations are discussed. The issues of methods and techniques of observations are touched upon. Several articles present the results of theoretical studies of phenomena and processes in plasma. The collection will be useful to specialists in the field of solar-terrestrial physics, graduate students and undergraduates.
76. Д7-90/84434
Исследования по физике Солнца : тезисы докладов всесоюзной конференции. – Ашхабад : Ылым, 1990. – 111 с. – ISBN 5-8338-0415-9. – В надзаг.: АН ТССР, Физ.-техн. ин-т. – Текст : непосредственный.
Abstract: Almost all priority areas of solar research are considered: the main mechanisms of solar activity; solar flares and unsteady processes; large-scale magnetic fields and differential rotation of the Sun; solar wind and interplanetary magnetic fields; the fine structure of the Sun's atmosphere; geoseismology and solar instruments. For specialists in the field of solar physics.
77. Ж2-21/70573
Киричек, Е. А. Неизвестное Солнце. Чудеса. Факты. Загадки. Расследование / Елена Киричек, Иван Панченко ; иллюстрации Марии Шишкану. – Якутск ; Москва : Айар, 2021. – 124, [3] с. : ил. – (Серия «Великий космос»). – ISBN 978-5-7696-6256-0. – Победитель конкурса «Книга года – 2021» в номинации Non-fiction. – Текст : непосредственный + Изображение (визуальное ; двухмерное) : непосредственное.
Abstract: The book, written by professional astrophysicists and has been scientifically edited at the Main (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences, contains unique and even fascinating material about our Sun star. It is written in cheerful language, beautifully illustrated and addressed to both schoolchildren and their parents. The book is the winner in the National Competition "Book of the Year – 2021" in the Non-fiction category, which is timed to coincide with the Year of Science and Technology announced by President Vladimir Putin. The competition was held with the support of the Ministry of Digital Development, Communications and Mass Communications of the Russian Federation.
78. Ж2-16/60602
Козлов, В. И. Аритмия Солнца. В космических лучах / В. И. Козлов, В. В. Козлов ; ответственный редактор Г. Ф. Крымский ; Институт космофизических исследований и аэрономии имени Ю. Г. Шафера Сибирского отделения Российской академии наук. – Якутск : Изд-во ФГБУН ИМЗ СО РАН, 2016. – 219 с. : ил. – Библиогр. в конце гл. – ISBN 978-5-93254-135-7. – Текст : непосредственный.
Abstract: The monograph is devoted to the study of transient solar wind regimes of various scales for the study of "group" features of the behavior of cosmic rays. It is established that the nonlocal properties of the magnetized medium, manifested in the correlation of cosmic ray fluctuations in the vicinity of the shock wave, can be used for its prediction with a lead time of ~ 1 day, and on large scales and ... the active phase of the solar cycle with a lead time of about ~ 1 solar revolution. This is due to the fact that the harbinger in cosmic rays is an indicator of the beginning of the restructuring of the magnetic field in the transition mode to the active phase of the solar cycle. Moreover, cosmic rays can provide valuable information about the possible development of the 11-year cycle for several years ahead. The book is addressed to both specialists in the field of cosmic rays and a wide range of readers interested in the problems of solar-terrestrial physics and is the Russian version of its translation into English.
79. М/66875/1
Колесник, А. Г. Солнечно-земная физика : учебное пособие / А. Г. Колесник. – Томск : ТМЛ-Пресс, 2010 – . – В надзаг.: Том. гос. ун-т. – Текст : непосредственный.
Ч. 1 : Солнце и межпланетная среда. – 2010. – 214 с. : ил. – Библиогр.: с. 205 (14 назв.). – ISBN 978-5-91302-117-5. – Текст : непосредственный.
Abstract: The book presents the first part of the textbook "Solar-Terrestrial physics", written by the author on the basis of a course of lectures given over a number of years to students and postgraduates of the Faculty of Radiophysics of Tomsk State University. The first part includes sections devoted to the physics of the Sun and the interplanetary medium. The author introduces the reader to the Sun as a star, its radiation spectrum, active formations on the Sun and solar activity, solar wind and interplanetary magnetic field, cosmic rays of various origin. The encyclopedic nature of the book, the simplicity and accessibility of the presentation, the author's ability to give a physical interpretation of the phenomena and processes under consideration, a rich and high–quality illustration of the material presented - all this should attract specialists, students and postgraduates working or interested in solar-terrestrial physics and related fields of science: radiophysics, geophysics, physical ecology, space physics.
80. М/16400/32 за 2021 г.
Колесниченко, А. В. Модифицированный в рамках негауссовой каппа-статистики интегральный критерий устойчивости Чандрасекара для равновесного сферического облака протозвезды / А. В. Колесниченко. – Москва : ИПМ им. М. В. Келдыша РАН, 2021. – 34 с. – (Препринт / Институт прикладной математики имени М. В. Келдыша Российской академии наук (Москва), ISSN 2071-2898 ; 32 за 2021 г.). – Загл. обл.: Модифицированный в рамках негауссовской каппа-статистики интегральный критерий устойчивости Чандрасекара для равновесного сферического облака протозвезды. – Библиогр.: с. 29-33. – DOI 10.20948/prepr-2021-32. – Текст : непосредственный.
Abstract: A generalization of Chandrasekhar's integral stability theorem of a spherically symmetric distribution of matter and black radiation in a protostellar cloud in a state of gravitational equilibrium is obtained within the framework of Kaniadakis' nonextensive statistical mechanics. For this purpose, the elements of deformed thermodynamics for an ideal gas, the deformed canonical Gibbs distribution, as well as the effective gravitational constant, calculations in the Verlinde formalism are used.
81. М/67453/29
Космические лучи / Международная академия оценки и консалтинга. – Москва : МАОК, 20 – . – Текст : непосредственный.
Т. 29 : Космические лучи и солнечная активность. – 2014. – 278 с. : ил. – Библиогр. в конце отд. ст. – ISBN 978-5-905114-14-4. – Текст : непосредственный.
Abstract: The collection presents the works of leading experts in the field of cosmic ray research and solar physics, in which an attempt is made to present the entire palette of cosmophysical research: from new instrumental research methods to theoretical research.
82. М/14715/1653
Кочаров, Г. Е. Термоядерный котел в недрах Солнца и проблема солнечного нейтрино / Г. Е. Кочаров. – Санкт-Петербург, 1995. – 22 c. : ил. – (Препринт / Физико-технический институт имени А. Ф. Иоффе (Ленинград) ; 1653). – Текст : непосредственный.
Abstract: The current state and prospects of the study of solar neutrinos, which are generated in the deep bowels of the Sun, are discussed.
83. М/14715/1461
Кочаров, Г. Е. Gamma-ray line solar flares catalogue, 1972-1986 / Г. Е. Кочаров, Yu. Yu. Kartavyh, G. A. Kovaltsov. – Leningrad, 1990. – 69 p. – (Препринт / Физико-технический институт имени А. Ф. Иоффе (Ленинград) ; 1461). – Перед загл. авт.: G. E. Kocharov, Yu. Yu. Kartavyh, G. A. Kovaltsov. – Bibliogr.: p. 54-69 (281 nazv.). – Текст : непосредственный.
Abstract: The catalog contains observational data on 58 solar flares with gamma-ray lines. It includes the characteristics of gamma radiation for these flares, data on solar cosmic rays, radio emission, as well as literature on these flares.
84. М/51525/4-96
Лубышев, Б. И. ССРТ : основные формулы для обработки данных наблюдений Солнца / Б. И. Лубышев, Т. А. Тресков. – Иркутск, 1996. – 52 с. : ил. – (Препринт / Институт солнечно-земной физики (Новосибирск) ; 4-96). – Текст : непосредственный.
Abstract: This preprint summarizes the main relationships that are necessary for processing the data of observations of the Sun obtained by the Siberian Solar Radio Telescope (SSRT).
85. Д9-07/51359
Лучков, Б. И. Наша звезда / Б. И. Лучков. – Москва : МИФИ, 2007 (Троицк (Моск. обл.)). – 98 с. : ил. – (Популярная физика). – Библиогр.: с. 97-98 (12 назв.). – ISBN 978-5-7262-0849-7. – В надзаг.: Моск. инженер.-физ. ин-т (гос. ун-т). – Текст : непосредственный.
Abstract: The book, intended for schoolchildren, students and teachers, is devoted to the physics of the Sun. It deals with the issues of the source of solar energy, the synthesis of elements in thermonuclear reactions occurring in the solar core, the evolution of the Sun, the manifestation of solar activity, the study of the Solar system. Both the fundamental, strictly established provisions of solar physics (thermonuclear reactions, the standard model of the Sun, cycles of solar activity) and the results of new research concerning the problem of solar neutrinos, the nature of solar flares, discoveries on the periphery of the Solar system are presented. A brief outline is given of solar (terrestrial and space) and thermonuclear energy (man-made Sun), which in the XXI century will replace thermal power plants as environmentally cleaner, inexhaustible and safe energy sources.
86. Ж2-03/31190
Магнитные поля и трехмерная структура солнечной атмосферы : всероссийская конференция, посвящённая 90-летию со дня рождения член-корреспондента Российской академии наук В. Е. Степанова. – Иркутск, 2003. – 57 с. : ил. – В надзаг.: Ин-т солнечно-земной физики СО РАН. – Библиогр. в конце отд. ст. – Текст : непосредственный.
Abstract: Large-scale magnetic fields of the sun. On the radiality of the magnetic field in the area of its measurement in a line according to the Kitt-Peak Observatory and calculations of the field in a potential approximation. About one forgotten effect of the solar dynamo theory. About one effect of the solar dynamo theory. Variations of the radius and quadrupole moment of the sun as a result of dynamo large-scale magnetic fields in the convective shell. Features of the spatial distribution of intensity ratios across the sun's disk in various combinations of spectral lines. Comparison of Sayan observations of the sun's magnetic fields with data from other observatories. Physical conclusions. Some results of studies of the magnetic field of the sun as a star based on stoksometric observations. Rotation of large-scale structures of solar activity by solar radio emission. Concepts and tasks of extrapolation of the field from photospheric observations. On the motion of plasma at the level of the photosphere in the magnetic field of the shadow of the spot. The structure of the magnetic field and electric currents in the chromosphere of active regions on the sun. Analysis of the helicity of the magnetic field of the active region. Instability of slow and fast waves of magnetic fields at different depths of the dynamo zone. Group-theoretic methods in solar physics. Investigation of the two-dimensional structure of the velocity field near quiet fibers at the Sayan Solar Observatory. On the structure of the magnetic field in the area of small solar flares. About the movements in the photosphere under active fibers. Evershed currents and oscillations. Flare-sympathetic magnetic structures on butterfly diagrams (vector representation) in cycles 17-22 of the sun and models of the flare process. On the relationship of the evolution of magnetic fields in the active region with the dynamics of powerful flares. On the type of wave of the fine structure of radio emission in the cm-band. Large-scale structure of chromospheric radial velocities on the sun's disk according to observations by two-dimensional spectroscopy. Anomalies of the chemical composition of the corona and the solar wind as a means to study the dynamics of the sun's atmosphere. Overview of modern ideas. Magnetic field and velocity field in the photosphere in the vicinity of fibers. Polarized radiation from Ellerman bombs or mustaches. Features of radio emission of coronal holes in the prilimbic regions. Evolutionary magnetic flux curves for slow and fast evolution. Cyclic variations of the contribution of the northern and southern hemispheres to the structure of the longitude inhomogeneity of solar activity. Shock linear polarization in solar flares. Features of the development of the chromospheric outbreak on October 19, 2001
87. Д8-94/16267
Магнитные поля Солнца и гелиосейсмология : сборник научных трудов / Российская академия наук, Физико-технический институт имени А. Ф. Иоффе ; редакционная коллегия: Дергачев В. А. (ответственный редактор) [и др.]. – Санкт-Петербург, 1994. – 188 c. : ил. – Библиогр.в конце отд.ст. – Текст : непосредственный.
Abstract: The traditional meeting of the working group "Solar cyclicity and forecasting of solar activity" of the section "The Sun" of the Astronomical Council of the Russian Academy of Sciences was held on May 12-23, 1994 at the Pulkovo Astronomical Observatory and was dedicated to the 80th anniversary of the birth of M. N. Gnedyshev. At the meetings of the group, 15 reports were heard related to the issues of solar activity research and solar-terrestrial relations. Most of the materials of the reports are presented in this collection on the problems of solar activity. This collection also includes part of the materials of the International Symposium on Solar-Terrestrial Physics, organized by the A. Navoi Samarkand State University with the active support of the Scientific Council of the Russian Academy of Sciences on the complex problem of "Solar-Terrestrial relations", in the period from October 13 to October 15, 1993.
88. Ж2-09/48156
Международная Байкальская молодежная научная школа по фундаментальной физике. Труды XI конференции молодых ученых «Гелио- и геофизические исследования» / Международная Байкальская молодежная научная школа по фундаментальной физике (2009 ; Иркутск). «Гелио- и геофизические исследования», конференция молодых ученых (11 ; 2009 ; Иркутск). – Иркутск, 2009 (Иркутск). – 365 с. : ил. – Библиогр. в конце ст. – В надзаг.: Ин-т солнечно-земной физики СО РАН, Иркут. гос. ун-т, Физ. фак. МГУ им. М. В. Ломоносова, Моск. физ.-техн. ин-т. – Текст : непосредственный.
Abstract: At the Conference of Young Scientists, reports were presented in the following areas: physics of near-Earth space; astrophysics and solar physics; interaction of radiation with matter; condensed states.
89. Ж2-07/42517
Многоволновые исследования Солнца и современные проблемы солнечной активности : труды всероссийской конференции, Специальная астрофизическая обсерватория, Российская академия наук, посёлок Нижний Архыз, Карачаево-Черкесская республика России, 28 сентября – 2 октября 2006 г. / Специальная астрофизическая обсерватория (Санкт-Петербург). – Санкт-Петербург : Спец. астрофиз. обсерватория, 2007 (СПб.). – 641 с. : ил. – В надзаг.: Рос АН, Спец. астрофиз. обсерватория, С.-Петерб. фил., Рос. фонд фундам. исслед., Астроном. о-во. – Текст : непосредственный.
Abstract: Presentation of the latest achievements in the field of experimental and theoretical studies of solar activity. Analysis of the maximum of 23 cycles of activity and the connection with the problem of "Space Weather". Main topics: magnetic fields in the Sun; oscillatory and cyclic processes in the Sun; solar corona research; active processes in the Sun; solar activity and disturbances of the solar wind and cosmic rays; modern observational methods of solar research; cooperative research programs of solar activity 2006-2007. Participation in the program "International Heliophysical Year".
90. Д1/31544
Мустель, Э. Р. Звездные атмосферы / Э. Р. Мустель ; редакционная коллегия: В. А. Амбарцумян [и др.]. – Москва : Гос. изд-во физ.-мат. литературы, 1960. – 444 с. : ил. ; 21 см. – (Проблемы теоретической астрофизики). – Библиогр.: с. 435-444 (204 назв.). – Текст : непосредственный.
Abstract: The issues related to the physical structure of stellar photospheres are considered and the analysis of absorption lines in the spectra of stars is given. Observations of the closest of them – the Sun – allowed us to establish that its atmosphere can be divided into a number of layers that differ from each other in their physical characteristics.
91. М/73441/5/3
Научные труды Института астрономии Российской академии наук = INASAN science reports / Институт астрономии (Москва). – Москва : Янус-К, 2019 – . – Парал. загл. англ. – ISSN 2658-5669. – Текст : непосредственный.
Т. 5, Вып. 3 / редакционная коллегия: М. Е. Сачков (главный редактор) [и др.]. – 2020. – С. 85-168 : ил. – Парал. загл. ст., аннот. англ. – Библиогр. в конце ст.
Abstract: Scientific Proceedings of the Institute of Astronomy of the Russian Academy of Sciences is a peer–reviewed journal that publishes articles on various aspects of astronomy, including theoretical and observational astrophysics, planetary astronomy, stellar astronomy, solar physics, celestial mechanics, astronomical methods and instruments, space research and research in the field of space geodesy.
92. М/24446/ПИЯФ-2011 2865
Новые ограничения на константу связи аксиона с электроном для аксионов, возникающих в результате тормозного излучения и комптоновского процесса на Солнце / А. В. Дербин [и др.]. – Гатчина, 2011. – 16 с. : ил. – (Препринт / Петербургский институт ядерной физики имени Б. П. Константинова ; ПИЯФ0-200-11 2865). – Библиогр.: с. 15-16 (38 назв.). – Текст : непосредственный.
Abstract: The search for the reaction of the acousto-electric effect in silicon atoms for solar axions arising as a result of bremsstrahlung and the Compton process is carried out. To register axions, a planar Si(Li) detector located in a low-background installation was used. As a result, a new model-independent restriction on the coupling constant of the axion with the electron |gAe| ≤ 2.2 10-10 is obtained, which leads to a restriction on the mass of the axion mA ≤ 7.9 eV and mA ≤ 1.4 keV in the DFSZ and KSVZ models of the axion, respectively (90% cu).
93. М/42146/143
Особенности временных изменений потоков S – компоненты Солнца на коротких волнах сантиметрового диапазона / О. А. Голубчина, С. Х. Тохчукова, В. М. Богод [и др.]. – Санкт-Петербург : [б. и.], 2003. – 54 с. : ил. – (Препринт / Специальная астрофизическая обсерватория (Ленинград) ; 143). – Библиогр.: с. 52-54 (15 назв.). – Текст : непосредственный.
Abstract: According to observations of the Sun's radio emission in the Southern sector of the RATAN-600 radio telescope on 11.09.01, the synchronicity of radiation from local sources (L. I.) was studied at waves of 1.92 cm, 2.24 cm, 2.74 cm and 3.21 cm. The dynamics of changes in L. I. fluxes with active processes in soft X–ray, On - flashes and bursts in the radio band at a frequency of 9100 MHz, the closest to the frequencies of our observations.
94. Н/13643/601
Петухов, М. Ю. Нелинейная генерация магнитно-акустико-гравитационных волн в атмосфере Солнца / М. Ю. Петухов, Ю. В. Петухов. – Нижний Новгород, 2001. – 23 с. : ил. – (Препринт / Институт прикладной физики (Нижний Новгород) ; 601). – Текст : непосредственный.
Abstract: Within the framework of a flat model of the isothermal atmosphere of the Sun permeated by a horizontal magnetic field, the intensity of which is proportional to the square root of the plasma density, and in the approximation of a given field for vertically propagating and non-propagating magneto-acoustic–gravitational waves, the regularities of nonlinear wave generation at difference and total frequencies, as well as acoustic flow (wind) - depending on depends on the magnitude of the magnetic field and the frequency of excitation of the initial disturbances at the lower boundary of the atmosphere.
95. М/24446/ПИЯФ-2006 2676
Поиск резонансного поглощения аксионов, излучаемых при М1-переходе в ядрах 57 Fe на Солнце / А. В. Дербин [и др.]. – Гатчина (Ленингр. обл.), 2006. – 19 с. – (Препринт / Ленинградский институт ядерной физики имени Б. П. Константинова ; ПИЯФ-2006 2676). – Библиогр.: с. 18-19 (30 назв.). – Текст : непосредственный.
Abstract: The resonant absorption of solar axions by 57Fe nuclei leading to the excitation of the first nuclear level: A+57Fe →57Fe*→57Fe + γ (14.4 keV) is searched for. A Si(Li) detector and a target made of the enriched isotope 57Fe were used to search for gamma quanta with an energy of 14.4 keV. The detector and the target were inside a low-background installation equipped with passive and active protection. As a result, a new upper limit on the mass of the axion mA≤ 360 eV (90{%} cu) was established.
96. Д10-16/33759
Попов, И. В. Стохастические процессы в физике явлений Земли и Солнца. Механизмы (принципы) / И. В. Попов. – Санкт-Петербург : Изд-во Политехн. ун-та, 2016. – 511 с. : ил. – Загл. обл.: Стохастические процессы в физике явлений Земли и Солнца. Механизмы. – Парал. тит. л. англ. – Библиогр.: с. 486-509. – ISBN 978-5-7422-5264-1. – Текст : непосредственный.
Abstract: The mechanisms of action of weak magnetic, electric and gravitational fields on various types of condensed media of the Earth, including its biological systems, and the mechanisms of occurrence of natural phenomena occurring on Earth and the Sun, including the influence of space weather, are described from a unified position. The root cause of all these manifestations is the internal fluctuation (stochastic) thermal field of their condensed media – electric and magnetic. The significance of a weak external permanent magnetic field as a factor controlling fluctuations of particles, their dynamic parameters and the internal thermal field of a condensed medium is determined. The internal field of the condensed media of the Earth and the Sun, together with their weak external dipole permanent magnetic field, participates in the formation of their own magnetic fields that determine their rotation. This internal field, together with the noise of magnetic, electric and gravitational fields (when the conditions of parametric generalized cyclotron resonance of condensed matter particles are met), is the source of the formation of vortex medium-stochastic magnetic fields and spiral vortices of the particles themselves. Vortex formation in the Sun is the cause of its activity, the reversal of magnetic fields in polar regions and sunspots, etc. And the properties of the high spectral density of the inhomogeneous stochastic internal thermal field determine the high temperature of the chromosphere and corona. On Earth, vortex formation is the cause of cyclones, tornadoes, earthquakes, etc. Everything goes according to the law of the Nature of the universe – chaos – order. The book is useful for those who are interested in the mechanisms of natural phenomena and how space weather affects them.
97. Ар20-2649
Поташов, М. Ш. Эффекты неравновесности и нестационарности в оболочках сверхновых : специальность 01.03.02 «Астрофизика и звёздная радиоастрономия» : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Поташов Марат Шамилевич. – Москва, 2020. – 22 с. : ил. – Библиогр.: с. 17-22. – Текст : непосредственный.
98. Ж2-01/27518
Пудовкин, М. И. Основы физики Солнца : курс лекций для бакалавров физического факультета / М. И. Пудовкин. – Санкт-Петербург, 2001. – 108 с. : ил. – ISBN 5-7997-0371-5. – В надзаг. С. -Петерб. гос. ун-т., Каф. физики Земли. – Текст : непосредственный.
Abstract: The course of lectures "Fundamentals of Solar Physics" is given to bachelors of the Faculty of Physics of St. Petersburg State University, specializing in the physics of Solar-terrestrial relations. The lectures cover the following issues: the main parameters of the Sun; sources of solar energy; the internal structure of the Sun and the structure of the solar atmosphere; Chapman's model of the solar corona and Parker's model of the expanding corona; solar wind; disturbed Sun, solar activity and its cycles, the connection of auroras, ionospheric, geomagnetic and magnetospheric disturbances with processes on the Sun.
99. Д1/22082
Северный, А. Б. Физика Солнца / А. Б. Северный ; ответственный редактор академик В. Г. Фесенков ; Академия наук СССР. – Москва : Изд-во Академии наук СССР, 1956. – 158, [1] с. : ил. – (Научно-популярная серия). – Библиогр.: с. 157 (5 назв.). – Текст : непосредственный.
Abstract: The Sun is considered as a cosmic body and its place in the Universe, the spectrum of the Sun and its interpretation. The physical structure of the Sun and the physical processes occurring on it are described. Attention is paid to the terrestrial manifestations of the processes occurring on the Sun.
100. Д8-97/36225
Современные проблемы солнечной цикличности : конференция, посвящённая памяти М. Н. Гневышева и А. И. Оля / Главная астрономическая обсерватория (Пулково). – Санкт-Петербург : Гл. астрон. обсерватория, 1997. – 427 с. : ил. – Библиогр. в конце докл. – Опис. по обл. без тит. л. – Текст : непосредственный.
Abstract: The reports of the participants of the conference "Modern problems of solar cyclicity" dedicated to the memory of M. N. Gnevyshev and A. I. Olya, held on May 26-30, 1997 in St. Petersburg, have been published.
101. М/55118/11/11
Солнечная активность и ее влияние на Землю : сборник статей. – Владивосток : Дальнаука, 20 – . – Текст : непосредственный.
Вып. 11. – 2008. – 146 с. : ил. – (Труды / Уссурийская астрофизическая обсерватория ; Т. 11). – Библиогр. в конце отд. ст. – ISBN 978-5-8044-0947-1.
Abstract: The collection contains articles devoted to various problems of solar physics: methods and results of measuring solar magnetic fields, statistical study of solar activity indices and solar flare dynamics, study of the interplanetary magnetic field, as well as the influence of solar and geomagnetic activity on the operation of marine navigation instruments. There are also articles on the method of measuring the radio flux of the Sun and the history of solar radio astronomy at the Ussuri Observatory. The collection of articles is intended for researchers and students specializing in the field of solar physics and solar-terrestrial relations.
102. М/55118/13(2010)
Солнечная активность и ее влияние на Землю : сборник статей / [редакционная коллегия: А. В. Баранов и др.]. – Владивосток : Дальнаука, 20 – . – Текст : непосредственный.
Вып. 13 (2010). – 2010. – 117 с. : ил. – (Ежегодник Уссурийской астрофизической обсерватории). – Библиогр. в конце ст. – ISBN 978-5-8044-1128-3.
Abstract: The articles devoted to the study of various aspects of solar physics are presented: methods and interpretation of measurements of solar magnetic fields, statistical characteristics of spot activity, eruptive processes in solar active regions, behavior of fluctuations of the interplanetary magnetic field. It is intended for researchers and students specializing in astronomy and geophysics, as well as for those who are interested in the impact of cosmic factors on the Earth.
103. М/55118/14
Солнечная активность и ее влияние на Землю : сборник статей. – Владивосток : Дальнаука, 20 – . – Текст : непосредственный.
Вып. 14. – 2011. – 118 с. – (Труды Уссурийской астрофизической обсерватории). – Библиогр. в конце ст. – ISBN 978-5-8044-1303-4.
Abstract: The collection contains articles on the physics of the Sun and the heliosphere. The articles describe the results of studies of the structure of the magnetic field and dynamic processes in solar active regions, long-term variations of solar activity, turbulence of the solar wind. The collection of articles is intended for researchers and students specializing in astronomy and geophysics, as well as for those interested in the impact of cosmic factors on the Earth.
104. Д10-15/28853
Солнечная и солнечно-земная физика – 2015 : 19-я всероссийская ежегодная конференция по физике Солнца : труды / Главная (Пулковская) астрономическая обсерватория. – Санкт-Петербург : Главная (Пулковская) астрономическая обсерватория РАН, 2015. – 401 с. : ил. – Рез. англ. – Библиогр. в конце отд. ст. – ISBN 978-5-9651-0935-7. – Текст : непосредственный.
Abstract: The topics of the conference included a wide range of issues on the physics of solar activity and solar-terrestrial relations. The conference was attended by scientists from the Russian Federation, Bulgaria, Poland, Great Britain, Finland, USA, Japan.
105. Н/17322/12(125)/1
Солнечно-земная физика : сборник научных трудов / Российская академия наук, Сибирское отделение, Институт солнечно-земной физики. – Иркутск : Изд-во Сиб. отд-ния Рос. АН, 20 – . – Текст : непосредственный.
Вып. 12(125), Т. 1 : Труды Международного симпозиума «Международный гелиофизический год – 2007 : новый взгляд на солнечно-земную физику», Звенигород, 5-11 ноября 2007 г. – 2008. – 195 с. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The symposium involves broad cooperation of scientists working in various fields of space research: physics of the Sun, heliosphere, magnetosphere, atmosphere, etc., for the possibility of studying the physical processes occurring in the Sun–Earth system as a single integral complex of phenomena. The holding of MGG - 2007 should contribute to the creation of global models linking phenomena occurring on the Sun with events in near-Earth space. The creation of such models is necessary to take into account the influence of the Sun and the near-Earth space environment on various technological systems, the Earth's climate, as well as on man himself. For this purpose, all available experimental data obtained in direct space experiments, as well as remote methods, should be used, and the efforts of theoretical scientists should be concentrated. The purpose of the symposium is to present and discuss the first results obtained under the MGG–2007 program and coordinate the implementation of further research in 2008. The main scientific topics of the symposium are: solar sources of geoeffective disturbances; the interplanetary medium – the medium of transmission of disturbances from the Sun to the Earth; the response of the magnetosphere, ionosphere and atmosphere to solar activity; climate, ecology and life.
106. У4543
Солнечно-земная физика = Solar-Terrestrial Physics / Институт солнечно-земной физики (Новосибирск). – Москва : ИНФРА-М, 2015 – (М.). – С № 3 за 2020 г. выходит только в электронном виде. – Выходит ежеквартально. – ISSN 2412-4737. – Текст : непосредственный.
Abstract: Main scientific areas of publications: theoretical and experimental studies of the Sun, solar activity and activity of solar-type stars; solar wind, interplanetary magnetic field; cosmic rays, their interaction with the heliosphere and the Earth's atmosphere; physical processes and phenomena occurring in near-Earth space; studies of the upper atmosphere, ionosphere and ionospheric propagation of radio waves; the influence of variations of solar energy and disturbances in the near-Earth environment on the functioning of ground-based and space-based technological systems; excitation and propagation of waves of various nature in near-Earth space; the role of solar and geomagnetic activity in the problems of seismicity, climate and biospheric processes; modeling, complex ground diagnostics and forecasting of space weather; lithospheric-atmospheric communications; scientific instrumentation (astrophysics and solar-terrestrial physics).
107. Солнечно-земная физика = Solar-Terrestrial Physics / Институт солнечно-земной физики (Новосибирск). – Москва : ИНФРА-М, 2015 – (М.). – С № 3 за 2020 г. выходит только в электронном виде. – Выходит ежеквартально. – ISSN 2712-9640. – URL: https://elibrary.ru/title_about_new.asp?id=7316 (дата обращения: 04.07.2022). – Access mode: Scientific Electronic Library eLIBRARY.RU. – Text : electronic.
Abstract: Main scientific areas of publications: theoretical and experimental studies of the Sun, solar activity and activity of solar-type stars; solar wind, interplanetary magnetic field; cosmic rays, their interaction with the heliosphere and the Earth's atmosphere; physical processes and phenomena occurring in near-Earth space; studies of the upper atmosphere, ionosphere and ionospheric propagation of radio waves; the influence of variations of solar energy and disturbances in the near-Earth environment on the functioning of ground-based and space-based technological systems; excitation and propagation of waves of various nature in near-Earth space; the role of solar and geomagnetic activity in the problems of seismicity, climate and biospheric processes; modeling, complex ground diagnostics and forecasting of space weather; lithospheric-atmospheric communications; scientific instrumentation (astrophysics and solar-terrestrial physics).
108. Д8-93/13484
Сомов, Б. В. Космическая электродинамика и физика Солнца / Б. В. Сомов. – Москва : Изд-во Моск. ун-та, 1993. – 287 c. : ил. – (Астрономия). – ISBN 5-211-02948-8. – В надзаг.: МГУ им. М. В. Ломоносова, Гос. астрон. ин-т им. П. К. Штернберга. – Библиогр.: с.281-287 (112 назв.). – Текст : непосредственный.
Abstract: An overview of some topical problems of space electrodynamics and solar physics is presented in their historical development and from the perspective of their discussion at the 16th school-seminar "Space Electrodynamics and Solar Physics", dedicated to the eightieth anniversary of the birth of S. I. Syrovatsky.
109. Д10-13/7805
Сотникова, Р. Т. Введение в гелиофизику : учебное пособие / Р. Т. Сотникова, В. Г. Файнштейн. – Иркутск : Изд-во ИГУ, 2013. – 256 с. : ил. – (Солнечно-земная физика). – Библиогр.: с. 205-208 (59 назв.). – ISBN 978-5-9624-0821-7. – В надзаг.: Иркут. гос. ун-т, Иркут. науч. центр СО РАН, Ин-т солнеч.-зем. физики. – Текст : непосредственный.
Abstract: The questions of the structure of the Sun, processes in the solar core, in the zone of radiant transport, in the convective region, in the solar atmosphere are considered. Modern results of studies of X-ray solar flares are given. The basic concepts of modern physics of the solar corona, including the large-scale structure of the corona and coronal mass ejections, are presented. The problems of corona heating and its cyclicity are touched upon. Various manifestations and cyclic patterns of solar activity are discussed. The important, and in many cases decisive, role of the magnetic field in solar processes is emphasized. The manual is intended for students, undergraduates and postgraduates specializing in astrophysics and solar physics.
110. Д10-13/8194
Сотникова, Р. Т. Рентгеновские вспышки на Солнце / Р. Т. Сотникова. – Иркутск : Изд-во ИГУ, 2013. – 142 с. : ил. – (Солнечно-земная физика). – Библиогр.: с. 121-142. – ISBN 978-5-9624-0875-0. – Текст : непосредственный.
Abstract: The influence of "space weather" factors on the geosphere determines the practical significance of research in this area. The most powerful manifestations of solar activity are flares. The proposed monograph contains an overview and results of studies of flares in the soft 1-8 Å X-ray range (GOES) for three cycles of solar activity (1977-2007). The findings are of interest both for the theory of flares and for the theory of dynamo. The book can be useful for students, undergraduates and postgraduates specializing in astrophysics and solar physics, as well as specialists engaged in solar research.
111. Ар14-3695
Стародубцев, С. А. Флуктуации интенсивности космических лучей в 11-летнем цикле солнечной активности : специальность 01.03.03 : автореферат диссертации на соискание учёной степени доктора физико-математических наук / Стародубцев С. А. – Якутск, 2014. – 56 с. : ил. – Библиогр.: с. 48-56 (56 назв.). – В надзаг.: Ин-т космофиз. исслед. и аэрономии им. Ю. Г. Шафера, Сиб. отд-ния Рос. акад. наук. – Текст : непосредственный.
112. Ж2-19/71232
Теоретические и программные средства анализа геофизических данных и выделения аномальных проявлений космической погоды / О. В. Мандрикова, Ю. А. Полозов, С. Ю. Хомутов [и др.] ; ответственный редактор Б. М. Шевцов ; Российская академия наук, Дальневосточное отделение, Институт космофизических исследований и распространения радиоволн. – Владивосток : Дальнаука, 2019. – 182, [1] с. : ил. – Библиогр.: с. 168-183 (244 назв.). – ISBN 978-5-8044-1690-5. – Текст : непосредственный.
Abstract: The monograph describes new methods of data analysis of geophysical monitoring systems. The field of research relates to the problems of the theory of processing direct experimental data and is related to monitoring and forecasting the state of near-Earth space. Special attention in the book is paid to methods of data analysis during periods of solar events, magnetic and ionospheric storms. The methods and computational algorithms developed by the authors are based on an integrated approach combining classical methods of data analysis and the latest scientific achievements in the field of pattern recognition and digital signal processing. An interactive software environment is described that implements storage, updating, provision to users and scientific analysis of recorded data from observation points of the ICIR FEB RAS. The book is intended for specialists engaged in research of processes in the field of solar-terrestrial physics, as well as specialists interested in modern achievements in the field of digital signal processing and analysis of direct experimental data.
113. Д10-13/8661
Теплицкая, Р. Б. Солнечная атмосфера : учебное пособие / Р. Б. Теплицкая. – Иркутск : Изд-во ИГУ, 2013. – 128 с. : ил. – (Солнечно-земная физика). – Библиогр.: с. 128 (16 назв.). – ISBN 978-5-9624-0878-1. – В надзаг.: Иркут. гос. ун-т, Сиб. отд-ние Рос. акад. наук, Ин-т солнеч.-зем. физики. – Текст : непосредственный.
Abstract: It is part of the interdisciplinary course "Solar-Terrestrial Physics", taught at the Institute of Solar-Terrestrial Physics SB RAI (ISSF) to graduate and undergraduates of the ISSF and Irkutsk State University. One of the sections of the course – "Solar atmosphere" is presented. It is assumed that the students are already familiar with the first two sections of the course: "Elements of plasma physics" and "Sun – star". The material is limited to information only about the calm sunny atmosphere. Chapters 1-3 of the manual give the basic, well-established concepts of the theory of radiation transfer, outline the principles of modeling the solar atmosphere, describe the most important processes occurring in the atmosphere of a calm Sun, as well as the principal features of optical instruments that diagnose the solar atmosphere. This part of the course is presented on the basis of "classical" textbooks and monographs published in previous years. The second part of the manual is based on the original articles, and can be revised in accordance with the further progress of solar astrophysics.
114. Н/341/4/2
Труды государственного астрофизического института / Астрофизический институт (Москва). – Москва : Книгосоюз, 19 – . – Текст : непосредственный.
Т. 4 : Результаты наблюдения полного солнечного затмения : 29-го июня 1927 г. в Мальмбергете (Швеция), Вып. 2. – 1929. – 80 с. + 7 л. ил. – Текст англ.
Abstract: The solar eclipse of June 29-th 1927 was observed by the expedition of the Russian Astrophysical Institute at Malmberget, Sweden. The site of observation, situated at the eastern extremity of the town, was about 10 kilometers to the north west of the line of central eclipse. The loss in the duration of totality amounted to 2 seconds, the calculated duration for Malmberget being 39,7 seconds. The following members took part in the expedition: B. Fessenkoff, G. Landsbergh, A. Michailov, K. Schistovsky and S. Vsessviatsky.
115. Н/8515/105
Физика магнитосферы, ионосферы и распространения радиоволн : сборник научных трудов / редакционная коллегия: Г. А. Жеребцов (главный редактор) [и др.]. – Новосибирск, 1997. – 239 с. : ил. – (Исследования по геомагнетизму, аэрономии и физике Солнца / Рос. АН, Сиб. отд-ние, Ин-т солнечно-зем. физики, ISSN 01353748 ; Вып. 105). – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The results of research on the physics of the magnetosphere and ionosphere are presented. In particular, some actual problems of physics of magnetospheric substorms are discussed. A number of articles are devoted to the analysis of short-period variations of the geomagnetic field, the study of energy particle flows in geostationary orbit, as well as processes in near-Earth space plasma. The issues of propagation of radio signals in the ionosphere, modeling and forecasting of the radio channel are considered.
116. Д10-16/37551
Физика солнечной плазмы и активность солнца : 17-я Международная солнечная конференция, 4-10 сентября 2016 г., [посёлок Научный, Крым] / Крымская астрофизическая обсерватория Российской академии наук ; [редакционная коллегия: Н. Н. Степанян и др.]. – Научный ; Симферополь : Антиква, 2016. – 91 с. – Текст рус., англ. – Библиогр. в конце некоторых ст. – ISBN 978-5-9908385-2-9. – Текст : непосредственный.
Abstract: The collection contains abstracts of reports submitted to the 17th International Solar Conference "Solar Plasma Physics and Solar Activity" (September 4-10, 2016, "KrAO RAS", Scientific, Crimea). The topics of the theses cover many topical issues of modern astrophysics and solar physics. The abstracts were published in the form in which they were presented by the authors, they were not edited, but were only brought to a single format. The collection is intended for specialists in the field of astronomy and astrophysics.
117. Д10-15/26255
Физика Солнца: теория и наблюдения : Международная конференция, посвященная 70-летию Крымской астрофизизической обсерватории, 6 – 12 сентября 2015 г., Научный – Симферополь : тезисы докладов / Крымская астрофизическая обсерватория [и др.]. – Симферополь : Антиква, 2015. – 95 с. : ил. – Библиогр. в конце отд. ст. – ISBN 978-5-9906277-7-2. – Текст : непосредственный.
Abstract: The International Conference "Solar Physics: Theory and Observations" was held from September 6 to 12, 2015 at the Crimean Astrophysical Observatory and was devoted to a wide range of issues on solar physics and solar-terrestrial relations. The scientific program of the conference included the following topics: chromosphere and corona research; structure and dynamics of solar formations. iii. Solar cycles. IV. The solar system and space weather. The conference was attended by 50 scientists from 7 countries (Russia, Great Britain, USA, Ukraine, Uzbekistan, Tajikistan, Kazakhstan). Russia was represented by participants from 19 scientific institutions. 59 reports were presented at the conference. This collection publishes the texts of reports submitted by the authors in the form of articles.
118. Ж2-06/39707
Физика Солнца и звезд : сборник трудов II Международного научного семинара «Физика Солнца и звезд», Элиста, 16-18 февраля 2005 г. / Калмыцкий государственный университет (Элиста) ; под редакцией Б. Б. Михаляева [и др.] – Элиста : Калмыц. ун-т, 2006 (Элиста). – 157 с. : ил. – Библиогр. в конце ст. – Текст : непосредственный.
Abstract: The book is a collection of the proceedings of the International Scientific Seminar "Physics of the Sun and Stars", held on February 16-18 at Kalmyk State University (Elista, Russia). The seminar was based on the work carried out in recent years by astrophysicists of Kalmyk and Volgograd State Universities, the Main (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences. The book is of interest to professional astronomers and physicists, graduate students and students of relevant specialties.
119. Ж2-06/41842
Физика Солнца и звезд : сборник трудов III Международного научного семинара, Элиста, 29 мая – 2 июня 2006 г. / Калмыцкий государственный университет (Элиста). – Элиста : КалмГУ, 2006. – 156 с. : ил. – Библиогр. в конце ст. – ISBN 5-230-20286-6. – В надзаг.: Калмыц. гос. ун-т. – Текст : непосредственный.
Abstract: The book is a collection of proceedings of the III International Scientific Seminar "Physics of the Sun and Stars", held on May 29 – June 2, 2006 at Kalmyk State University (Elista, Russia). The seminar was based on the work carried out by astrophysicists of the Kalmyk and Volgograd Universities, as well as the Main (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences. The book is of interest to professional astronomers and physicists, graduate students and students of relevant specialties.
120. Ж2-08/45918
Физика Солнца и звезд : сборник трудов IV Всероссийского научного семинара «Физика Солнца и звезд», Элиста (Россия), 22 – 25 апреля 2008 г. / Калмыцкий государственный университет (Элиста) ; под редакцией Б. Б. Михаляева [и др.]. – Элиста : КалмГУ, 2008. – 157 с. : ил. – Библиогр. в конце докл. – ISBN 978-5-91458-046-6. – В надзаг.: Рос. фонд фундам. исслед., ГОУ ВПО «Калмыц. гос. ун-т». – Текст : непосредственный.
Abstract: The book is a collection of the proceedings of the All-Russian scientific seminar "Physics of the Sun and Stars", held on April 22-25 at Kalmyk State University (Elista, Russia). The seminar was based on the work carried out by astrophysicists of the Kalmyk and Volgograd Universities, as well as the Main (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences. The book is of interest to professional astronomers and physicists, graduate students and students of relevant specialties.
121. Ж2-13/57930
Физика Солнца и околоземного космического пространства : труды Всероссийской конференции по солнечно-земной физике, посвященной 100-летию со дня рождения В. Е. Степанова, Иркутск, 16-21 сентября 2013 г. – Иркутск : Ин-т солнеч.-зем. физики, 2013. – 309 с. : ил. – Библиогр. в конце отд. ст. – Текст : непосредственный.
Abstract: The proceedings of the All-Russian Conference on Solar-Terrestrial Physics dedicated to the 100th anniversary of the birth of Corresponding member of the Russian Academy of Sciences V. E. Stepanov (Irkutsk, September 16-21, 2013) are published in the collection. The collection opens with articles about the scientific activities of V. E. Stepanov. The results of studies of solar magnetic fields, processes in the solar atmosphere and heliosphere are presented. Special attention is paid to the results of studies of the entire chain of solar-terrestrial relations: from the occurrence of disturbances in the Sun, their propagation in the interplanetary medium and direct impact on the magnetosphere, atmosphere and climate of the Earth. The developments of new instruments and research methods in solar-terrestrial physics are presented. The collection is of interest to specialists in the field of solar-terrestrial physics and related fields of knowledge, graduate students and undergraduates of relevant specialties.
122. М/14605/ИТФ-90-4Р
Харченко, Н. В. Пространственные и эволюционные характеристики звезд в окрестностях Солнца / Н. В. Харченко. – Киев, 1990. – 17 с. – (Препринт / Институт теоретической физики (Киев) ; ИТФ-90-4Р). – Библиогр.: с. 15-17 (30 назв.). – Текст : непосредственный.
Abstract: Based on the data from the catalog of astronomical characteristics of the stars of the program of the meridional section of the Galaxy and long-period variables, it is obtained that the stars of great age are located in the vicinity of the Sun in the form of a fragment of a spiral arm. The magnitude of the gradients of the evolutionary characteristics in the direction perpendicular to the axis of the sleeve is determined. These gradients have opposite signs for young (supergiants of luminosity classes I and II) and old stars.
123. Ар19-2059
Хлыстова, А. И. Течения плазмы при появлении активных областей в фотосфере Солнца : специальность 01.03.03 «Физика Cолнца» : автореферат диссертации на соискание учёной степени кандидата физико-математических наук / Хлыстова А. И. ; Институт солнечно-земной физики Сибирского отделения Российской академии наук. – Иркутск, 2019. – 20 с. : ил. – Библиогр.: с. 19-20. – Текст : непосредственный.
124. М/55118/1
Чистяков, В. Ф. Солнечные циклы и колебания климата / В. Ф.Чистяков. – Владивосток : Дальнаука, 1997. – 155 с. : ил. – (Труды / Уссурийская астрофизическая обсерватория ; вып. 1). – Библиогр.: с. 138-154 (411 назв.). – Текст : непосредственный.
Abstract: The monograph considers the issue of finding solar activity cycles based on astronomical observations and their influence on the earth's climate. In addition to 11-year fluctuations, those with a longer period (2,400 years or more) and their impact on the development of mankind are also considered. For climatologists and solar researchers.
125. Д9-11/83047
Язев, С. А. Лекции о солнечной системе : учебное пособие / С. А. Язев; под редакцией В. Г. Сурдина. – 2-е изд., испр. и доп. – Санкт-Петербург [ и др.] : Лань, 2011 (Архангельск). – 384 с. : ил. – (Учебники для вузов. Специальная литература). – Библиогр.: с. 379-381. – ISBN 978-5-8114-1253-2. – Текст : непосредственный.
Abstract: Two thousand years ago, the Sun was a character of many legends, a mythical spirit or even a god. For a long time it was believed that the sun of day moves around the center of the world – the Earth. Four hundred years ago, people looked at the Sun through the first telescopes – and could not believe what they saw. Today, the Sun is studied by several thousand specialists, but what do we know about it? How did we get this knowledge? This book is not only about the Sun itself, but also about our ideas about it. About how speculative reasoning was replaced by scientific hypotheses, and old hypotheses were replaced by new ones. About how to study what is impossible to touch, and why such knowledge is reliable. About how difficult and dramatic the path of the explorers of the Sun can be. And, of course, about all the most interesting things that are happening on our star.
126. Д10-14/20876
Язев, С. А. Феномен комплексов активности на Солнце / С. А. Язев ; Иркутский государственный университет [и др.]. – Иркутск : Изд-во ИГУ, 2014. – 377 с. : ил. – Библиогр.: с. 337-356 (394 назв.). – ISBN 978-5-9624-1089-0. – Текст : непосредственный.
Abstract: The monograph is devoted to the study of long-lived large-scale magnetic formations on the Sun, called activity complexes. The results of the study of the morphology, statistics and evolution of activity complexes obtained for the most part by the author and his co-authors are presented, the question of solar flares associated with activity complexes is considered, a phenomenological model of the activity complex is presented. The publication is intended for researchers, postgraduates and undergraduates of physical specialties of universities, as well as all specialists interested in solar and solar-terrestrial physics.
127. Degl'Innocenti E. L. Fisica solare / E. L. Degl'Innocenti. – Electronic text data. – Milano : Springer-Verlag, 2008. – 293 p. – ISBN 978-88-470-0678-2. – URL: http://dx.doi.org/10.1007/978-88-470-0678-2 (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: Il volume è un'introduzione alla Fisica Solare che si propone lo scopo di illustrare alla persona che intende avvicinarsi a questa disciplina (studenti, dottori di ricerca, ricercatori) i meccanismi fisici che stanno alla base della complessa fenomenologia osservata sulla stella a noi più vicina. Il volume non ha la pretesa di essere esauriente (basta pensare che la fisica solare spazia su un gran numero di discipline, quali la Fisica Nucleare, la Termodinamica, L'Elettrodinamica, la Fisica Atomica e Molecolare, la Spettoscopia in tutte le bande dello spettro elettromagnetico, la Magnetoidrodinamica, la Fisica del Plasma, lo sviluppo di nuova strumentazione, l'Ottica, ecc.). Piuttosto, sono stati scelti un numero di argomenti di rilevanza fondamentale nello studio presente del Sole (soprattutto nei riguardi delle osservazioni da terra con grandi telescopi) e su tali argomenti si è cercato di dare una panoramica generale, inclusiva dell'evoluzione storica, senza scendere in soverchi dettagli. Siccome la Fisica Solare può a buon diritto essere considerata la «Stele di Rosetta» di tutta l'Astrofisica, il volume può anche essere considerato una valida introduzione a questa materia.
128. R/6714/153
Energetic phenomena on the sun : a result of three meet., Goddard space flight center, January 24-28, 1983, June 8-14, 1984, February 13-17, 1984 / editor M. R. Kundu. – Dordrecht [etc.] : Kluwer, 1989. – XXVIII, 632 p. – 632 p. : ill. – (Astrophysics and space science library / Ed.: J. E. Blamont ; vol.153). – ISBN 0-7923-0129-3. – Библиогр. в конце гл. – Указ.: с.615-625. – Текст : непосредственный.
Abstract: This publication is a result of three meetings, each 5 days long, held at the Goddard Space Flight Center on January 24-28, 1983, June 8-14, 1983, and February 13-17, 1984. The meetings were held in the interim between the full operations of the Solar Maximum Mission (SMM) in 1980, and the renewed operations after its repair in orbit in April 1984. Their general objectives were as follows: o Synthesize flare studies after three years of SMM data analysis. Many analyses of individual flares and individual phenomena, often jointly across many data sources had been published, but a need existed for a broader synthesis and updating of our understanding of solar flares since the Skylab Flare Workshops held several years earlier. o Encourage a broader participation in the SMM data analysis and combine this more fully with theory and other data sources--data obtained with other spacecraft such as the HINOTORI, P78-1, and ISEE-3 spacecrafts, and with the Very Large Array (VLA) and many other ground-based instruments. Many coordinated data sets, unprecedented in their breadth of coverage and multiplicity of sources, had been obtained within the structure of the Solar Maximum Year (SMY). Stimulate joint studies, and publication in the general scientific literature. The intended primary benefit was for informal collaborations to be started or broadened at the Workshops with subsequent publications. Provide a special publication resulting from this Workshop. Provide a starting point of understanding for planning renewed full observations with the repaired SMM.
129. Helioseismology, asteroseismology, and MHD connections / editor L. Gizon. – Electronic text data. – Berlin ; Heidelberg : Springer, 2009. – 637 p. – ISBN 978-0-387-89482-9. – URL: http://dx.doi.org/10.1007/978-0-387-89482-9 (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: This volume presents a timely snapshot of the state of helio- and asteroseismology in the era when the SOHO/MDI instrument is about to be replaced by SDO/HMI and the CoRoT space mission is yielding its first long-duration light curves of thousands of stars. The articles and topics in this book are inspired by two seminal conferences, HELAS II and SOHO19/GONG 2007, but contributions from other experts have been commissioned as well. For example, three key papers were invited to describe the current status of asteroseismology, global helioseismology, and local helioseismology. These papers provide a framework for the other contributions and together they form a complete description of our understanding of pressure waves in the Sun and other stars. This volume is aimed at solar physicists and astronomers specializing in helio- and asteroseismology.
130. R/6714/159
Inside the Sun : proceedings of the 121st colloquium of the international astrophysical union, May 22-26, 1989, Versailles / International astronomical union ; editor G. Berthomieu, M. Cribier. – Dordrecht [etc.] : Kluwer, 1990. – XI, 518 p. – 518 p. : ill. – (Astrophysics and space science library / Ed.: J. E. Blamont ; vol.159). – ISBN 0-7923-0662-7. – Библиогр. в конце ст. – Указ.: с.497-513. – Текст : непосредственный.
Abstract: Inside the Sun: Unsolved Problems. 1: Solar Modelling. – The Standard Solar Model. – Equation of State and Ionization of Dense Plasmas. – Nuclear Reactions in the Sun. – Solar Opacities Constrained by Solar Neutrinos and Solar Oscillations. – Astrophysical Opacities at LLNL. – Constraints on Solar Models from Stellar Evolution. – Convection in the Sun. – Comments on Solar Convection. – On the Accuracy of Solar Modelling. – A Look on Non-standard Solar Models. – Solar Cosmions. – L'isotope 3He dans les etoiles. Application a la theorie des Novae et des naines blanches. 2: Neutrinos. – Solar Neutrino Projects. – Report on the Homestake Chlorine Solar Neutrino Experiment. – The Kamiokande Solar Neutrino Experiment. – The GALLEX Project. – The Baksan Gallium Solar Neutrino Experiment. – Neutrino Masses, Neutrino Oscillations and Dark Matter. – Matter Effects in Neutrino Propagation. 3: Helioseismology. – A Review of Observational Helioseismology. – Networks for Helioseismic Observations.- Recent Helioseismological Results from Space. – Future Prospects of Helioseismology from Space. – Helioseismic Investigation of Solar Internal Structure. – Using Helioseismic Data to Probe the Hydrogen Abundance in the Solar Core. – Magnetic Field in the Sun's Interior from Oscillation Data. – Variations of the Low I Solar Acoustic Spectrum Correlated with the Activity Cycle. – Stellar Seismology. – Solar and Stellar Cycles. 4: Solar Cycle, Dynamo and Transport Processes. – The Solar Dynamo. – The Evolution of the Sun's Angular Momentum. – Angular Momentum Transport and Magnetic Fields in the Solar Interior. – Theory of Transport Processes. – Surface Abundances of Light Elements as Diagnostic of Transport Processes in the Sun and Solar-type stars.
131. Proceedings of the third un/esa/nasa workshop on the international heliophysical year 2007 and basic space science : national astronomical observatory of Japan / editor H. J. Haubold. – Electronic text data. – Berlin ; Heidelberg : Springer, 2010. – (Astrophysics and space science proceedings, ISSN 1570-6591). – ISBN 978-3-642-03325-4. – URL: http://dx.doi.org/10.1007/978-3-642-03325-4 (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: This book represents Volume II of the Proceedings of the UN/ESA/NASA Workshop on the International Heliophysical Year 2007 and Basic Space Science, hosted by the National Astronomical Observatory of Japan, Tokyo, 18 – 22 June, 2007. It covers two programme topics explored in this and past workshops of this nature: non-extensive statistical mechanics as applicable to astrophysics, addressing q-distribution, fractional reaction and diffusion, and the reaction coefficient, as well as the Mittag-Leffler function and the TRIPOD concept, developed for astronomical telescope facilities.
132. Putting the «I» in IHY : the United Nations report for the international heliophysical year 2007 / editor B. J. Thompson [et al.]. – Electronic text data. – Vienna : Springer, 2009. – 371 p. – (Studies in space policy, ISSN 1868-5307). – ISBN 978-3-211-99180-0. – URL: http://dx.doi.org/10.1007/978-3-211-99180-0 (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: Putting the «I» in IHY This book is about international cooperation. It demonstrates how the power of scientist imagination and investigation can bring together people form all continents in almost all countries around the globe. In presenting this impressive result, we can understand, how much unifying force the quest for understanding our universe and using outer space for that purpose have. Astronomy is far away from being a «political» area of science. But is has enormous political effects – and all of these effects are positive. This book about the international aspects and achievements of the «International Heliophysical Year (IHY) 2007» can be regarded as a compendium of the fertile impacts of conducting research in this eld. The main focus, as the title implicates, is the international cooperation, which has emerged from this grassroots initiative. North and South, industrialized and developing countries have been coordinating their efforts and have been learning from each other in a mutual partnership under a joint understanding of sharing the scientist benets. Through this, trans-border networks have been created and scientist as well as cultural exchange took place.
133. Solar Physics. – Electronic text data. – Berlin : Springer Science+Business Media, 1967 – (Springer). – ISSN 0038-0938. – URL: https://www.springer.com/journal/11207/aims-and-scope (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Articles on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun. That is, results of solar−terrestrial physics are included if they are clearly related to the physics of the Sun or if they use terrestrial phenomena as indicators of solar activity. Articles on stellar research as long as their results have a direct impact upon the understanding of the Sun, its structure and activity, or when solar observations are used when interpreting stellar data. Proceedings of conferences are not published in Solar Physics. However, some issues of the journal may be Topical Issues which are concerned with a specific topic selected by the editors and, in some cases, may contain papers presented at a monothematic conference. All papers submitted to such a collection are handled and refereed in the same way as regular research papers. Contrary to proceedings, the length of such papers is not limited, and other papers related to the same topic, not presented at the conference, can be added to the issue.
134. R/12125/344
Solar physics and astrophysics at interferometric resolution : proceedings of an ESA workshop on solar physics and astrophysics at interferometric resolution, Paris, February 17-19, 1992 / editor L. Dame, T. -D. Guyenne. – Paris : ESA, 1992. – 322 p. : ill. – (Special publication / Europ. space agency ; n 344). – ISBN 92-9092-218-4. – Библиогр. в конце статей. – Текст : непосредственный.
Abstract: Session 1: Very High Resolution Solar Physics; Session 2: Solar System & Galactic Astrophysics at High Resolution; Session 3: SIMURIS Model Payloads – Instrumentation & Performances; Session 4: Strategy for Interferometry from Space.
135. The hinode mission / editor T. Sakurai. – Electronic text data. – New York, NY : Springer, 2009. – 207 p. – ISBN 978-0-387-88739-5. – URL: https://doi.org/10.1007/978-0-387-88739-5 (дата обращения: 05.07.2022). – Access mode: for authorization. users.
Abstract: The Solar-B satellite was launched in the morning of 23 September 2006 (06:36 Japan time) by the Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), and was renamed to Hinode (‘sunrise’ in Japanese). Hinode carries three instruments; the X-ray telescope (XRT), the EUV imaging spectrometer (EIS), and the solar optical telescope (SOT). These instruments were developed by ISAS/JAXA in cooperation with the National Astronomical Observatory of Japan as domestic partner, and NASA and the Science and Technology Facilities Council (UK) as international partners. ESA and Norwegian Space Center have been providing a downlink station. All the data taken with Hinode are open to everyone since May 2007.
136. R/9392/373
<The>sun: a laboratory for astrophysics : proceedings of the NATO advanced study institute on the sun, Crief, June 16-29, 1991 / editor J. T. Schmelz, J. C. Brown. – Dordrecht [etc.] : Kluwer, 1992. – 617 p. : ill. – (NATO advanced study institute series. Ser. C, Mathematical and physical sciences ; vol. 373). – ISBN 0-7923-1811-0. – Указ.: с. 601-617. – Текст : непосредственный.
Abstract: As in the days following Skylab, solar physics came to the end of an era when the Solar Maximum Mission re-entered the earth's atmosphere in December 1989. The 1980s had been a pioneering decade not only in space- and ground-based studies of the solar atmosphere (Solar Maximum Mission, Hinotori, VLA, Big Bear, Nancay, etc.) but also in solar-terrestrial relations (ISEE, AMPTE), and solar interior neutrino and helioseismology studies. The pace of development in related areas of theory (nuclear, atomic, MHD, beam-plasma) has been equally impressive. All of these raised tantalizing further questions about the structure and dynamics of the Sun as the prototypical and best observed star. This Advanced Study Institute was timed at a pivotal point between that decade and the realisation of Yohkoh, Ulysses, SOHO, GRANAT, Coronas, and new ground-based optical facilities such as LEST and GONG, so as to teach and inspire the up and coming young solar researchers of the 1990s. The topics, lecturers, and students were all chosen with this goal in mind, and the result seems to have been highly successful by all reports.
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