Physical Processes in Solar Flares:
Gespeichert in:
1. Verfasser: | |
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Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Dordrecht
Springer Netherlands
1992
|
Schriftenreihe: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
172 |
Schlagworte: | |
Online-Zugang: | Volltext |
Beschreibung: | Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists |
Beschreibung: | 1 Online-Ressource (VIII, 249 p) |
ISBN: | 9789401123969 9789401050562 |
ISSN: | 0067-0057 |
DOI: | 10.1007/978-94-011-2396-9 |
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Datensatz im Suchindex
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any_adam_object | |
author | Somov, Boris V. |
author_facet | Somov, Boris V. |
author_role | aut |
author_sort | Somov, Boris V. |
author_variant | b v s bv bvs |
building | Verbundindex |
bvnumber | BV042415858 |
classification_tum | PHY 000 |
collection | ZDB-2-PHA ZDB-2-BAE |
ctrlnum | (OCoLC)863753054 (DE-599)BVBBV042415858 |
dewey-full | 523.01 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 523 - Specific celestial bodies and phenomena |
dewey-raw | 523.01 |
dewey-search | 523.01 |
dewey-sort | 3523.01 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
doi_str_mv | 10.1007/978-94-011-2396-9 |
format | Electronic eBook |
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id | DE-604.BV042415858 |
illustrated | Not Illustrated |
indexdate | 2024-07-10T01:20:58Z |
institution | BVB |
isbn | 9789401123969 9789401050562 |
issn | 0067-0057 |
language | English |
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physical | 1 Online-Ressource (VIII, 249 p) |
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series2 | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |
spelling | Somov, Boris V. Verfasser aut Physical Processes in Solar Flares by Boris V. Somov Dordrecht Springer Netherlands 1992 1 Online-Ressource (VIII, 249 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 172 0067-0057 Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists Physics Astrophysics and Astroparticles Plasmaphysik (DE-588)4046259-6 gnd rswk-swf Flare (DE-588)4277650-8 gnd rswk-swf Flare (DE-588)4277650-8 s Plasmaphysik (DE-588)4046259-6 s 1\p DE-604 https://doi.org/10.1007/978-94-011-2396-9 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
spellingShingle | Somov, Boris V. Physical Processes in Solar Flares Physics Astrophysics and Astroparticles Plasmaphysik (DE-588)4046259-6 gnd Flare (DE-588)4277650-8 gnd |
subject_GND | (DE-588)4046259-6 (DE-588)4277650-8 |
title | Physical Processes in Solar Flares |
title_auth | Physical Processes in Solar Flares |
title_exact_search | Physical Processes in Solar Flares |
title_full | Physical Processes in Solar Flares by Boris V. Somov |
title_fullStr | Physical Processes in Solar Flares by Boris V. Somov |
title_full_unstemmed | Physical Processes in Solar Flares by Boris V. Somov |
title_short | Physical Processes in Solar Flares |
title_sort | physical processes in solar flares |
topic | Physics Astrophysics and Astroparticles Plasmaphysik (DE-588)4046259-6 gnd Flare (DE-588)4277650-8 gnd |
topic_facet | Physics Astrophysics and Astroparticles Plasmaphysik Flare |
url | https://doi.org/10.1007/978-94-011-2396-9 |
work_keys_str_mv | AT somovborisv physicalprocessesinsolarflares |