The Solar Chromosphere and Corona: Quiet Sun:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1976
|
| 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
53 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The widespread tendency in solar physics to divide the solar atmosphere into separate layers and to distinguish phenomena of solar activity from phenomena of the quiet Sun emphasizes the wide ranging diversity of physical conditions and events occurring in the solar atmosphere. This diversity spans the range from a neutral, essentially quiescent atmosphere to a highly ionized, violently convective atmosphere; from a domain in which magnetic field effects are unimportant to a domain in which the magnetic pressure exceeds the gas pressure, and from a domain in which the particle motions are Maxwellian to a domain in which an appreciable fraction of the particles is accelerated to relativistic energies. It is now widely recognized that the chromosphere and corona have a common origin in the mechanical energy flux generated in the hydrogen convection zone lying beneath the photosphere. Furthermore, magnetic field phenomena appear to be as vital to the structure of th~ quiet Sun as to the active Sun. For these reasons it appears desirable to present a unified treatment of the entire solar atmosphere, both active and quiet, in a single volume. On the other hand, such a treatise must be very long if it is to avoid being superficial, and it is very difficult for a single author to write authoritatively on such a wide range of topics |
| Beschreibung: | 1 Online-Ressource (515p) |
| ISBN: | 9789401017152 9789401017176 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-010-1715-2 |
Internformat
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| 245 | 1 | 0 | |a The Solar Chromosphere and Corona: Quiet Sun |c by R. Grant Athay |
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| 500 | |a The widespread tendency in solar physics to divide the solar atmosphere into separate layers and to distinguish phenomena of solar activity from phenomena of the quiet Sun emphasizes the wide ranging diversity of physical conditions and events occurring in the solar atmosphere. This diversity spans the range from a neutral, essentially quiescent atmosphere to a highly ionized, violently convective atmosphere; from a domain in which magnetic field effects are unimportant to a domain in which the magnetic pressure exceeds the gas pressure, and from a domain in which the particle motions are Maxwellian to a domain in which an appreciable fraction of the particles is accelerated to relativistic energies. It is now widely recognized that the chromosphere and corona have a common origin in the mechanical energy flux generated in the hydrogen convection zone lying beneath the photosphere. Furthermore, magnetic field phenomena appear to be as vital to the structure of th~ quiet Sun as to the active Sun. For these reasons it appears desirable to present a unified treatment of the entire solar atmosphere, both active and quiet, in a single volume. On the other hand, such a treatise must be very long if it is to avoid being superficial, and it is very difficult for a single author to write authoritatively on such a wide range of topics | ||
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Datensatz im Suchindex
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| author | Athay, R. Grant |
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| author_sort | Athay, R. Grant |
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| bvnumber | BV042415564 |
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| 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 | 10.1007/978-94-010-1715-2 |
| format | Electronic eBook |
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| geographic_facet | Sonne Sonnenkorona |
| id | DE-604.BV042415564 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789401017152 9789401017176 |
| issn | 0067-0057 |
| language | English |
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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 | Athay, R. Grant Verfasser aut The Solar Chromosphere and Corona: Quiet Sun by R. Grant Athay Dordrecht Springer Netherlands 1976 1 Online-Ressource (515p) 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 53 0067-0057 The widespread tendency in solar physics to divide the solar atmosphere into separate layers and to distinguish phenomena of solar activity from phenomena of the quiet Sun emphasizes the wide ranging diversity of physical conditions and events occurring in the solar atmosphere. This diversity spans the range from a neutral, essentially quiescent atmosphere to a highly ionized, violently convective atmosphere; from a domain in which magnetic field effects are unimportant to a domain in which the magnetic pressure exceeds the gas pressure, and from a domain in which the particle motions are Maxwellian to a domain in which an appreciable fraction of the particles is accelerated to relativistic energies. It is now widely recognized that the chromosphere and corona have a common origin in the mechanical energy flux generated in the hydrogen convection zone lying beneath the photosphere. Furthermore, magnetic field phenomena appear to be as vital to the structure of th~ quiet Sun as to the active Sun. For these reasons it appears desirable to present a unified treatment of the entire solar atmosphere, both active and quiet, in a single volume. On the other hand, such a treatise must be very long if it is to avoid being superficial, and it is very difficult for a single author to write authoritatively on such a wide range of topics Physics Astrophysics and Astroparticles Chromosphäre (DE-588)4258764-5 gnd rswk-swf Sonne (DE-588)1236963652 gnd rswk-swf Sonnenkorona (DE-588)4181832-5 gnd rswk-swf Sonne (DE-588)1236963652 g Chromosphäre (DE-588)4258764-5 s Sonnenkorona (DE-588)4181832-5 g 1\p DE-604 https://doi.org/10.1007/978-94-010-1715-2 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Athay, R. Grant The Solar Chromosphere and Corona: Quiet Sun Physics Astrophysics and Astroparticles Chromosphäre (DE-588)4258764-5 gnd |
| subject_GND | (DE-588)4258764-5 (DE-588)1236963652 (DE-588)4181832-5 |
| title | The Solar Chromosphere and Corona: Quiet Sun |
| title_auth | The Solar Chromosphere and Corona: Quiet Sun |
| title_exact_search | The Solar Chromosphere and Corona: Quiet Sun |
| title_full | The Solar Chromosphere and Corona: Quiet Sun by R. Grant Athay |
| title_fullStr | The Solar Chromosphere and Corona: Quiet Sun by R. Grant Athay |
| title_full_unstemmed | The Solar Chromosphere and Corona: Quiet Sun by R. Grant Athay |
| title_short | The Solar Chromosphere and Corona: Quiet Sun |
| title_sort | the solar chromosphere and corona quiet sun |
| topic | Physics Astrophysics and Astroparticles Chromosphäre (DE-588)4258764-5 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Chromosphäre Sonne Sonnenkorona |
| url | https://doi.org/10.1007/978-94-010-1715-2 |
| work_keys_str_mv | AT athayrgrant thesolarchromosphereandcoronaquietsun |