Coronal Expansion and Solar Wind:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Berlin, Heidelberg
Springer Berlin Heidelberg
1972
|
| Schriftenreihe: | Physics and Chemistry in Space
5 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Little more than ten years have passed since spaceprobe-borne instruments con clusively demonstrated the existence of the solar wind. These observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interplanetary plasma near the orbit of the earth are now known in great detail. The theory of the coronal ex pansion has also been highly refilled both in the sense of including additional physical processes, and of treating more realistic (time-dependent and non spheri cally-symmetric) coronal boundary conditions. The present volume is an attempt to synthesize the solar wind observations and coronal expansion models from this decade of rapid development. The ultimate goal is, of course, the interpretation of observed solar wind phenomena as the effects of basic physical processes occurring in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "large-scale" features revealed by the observations. It requires extensive use of the concepts and methods of fluid mechanics |
| Beschreibung: | 1 Online-Ressource (XII, 238 p) |
| ISBN: | 9783642654145 9783642654169 |
| ISSN: | 0079-1938 |
| DOI: | 10.1007/978-3-642-65414-5 |
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| discipline | Physik |
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| spelling | Hundhausen, A. J. Verfasser aut Coronal Expansion and Solar Wind by A. J. Hundhausen Berlin, Heidelberg Springer Berlin Heidelberg 1972 1 Online-Ressource (XII, 238 p) txt rdacontent c rdamedia cr rdacarrier Physics and Chemistry in Space 5 0079-1938 Little more than ten years have passed since spaceprobe-borne instruments con clusively demonstrated the existence of the solar wind. These observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interplanetary plasma near the orbit of the earth are now known in great detail. The theory of the coronal ex pansion has also been highly refilled both in the sense of including additional physical processes, and of treating more realistic (time-dependent and non spheri cally-symmetric) coronal boundary conditions. The present volume is an attempt to synthesize the solar wind observations and coronal expansion models from this decade of rapid development. The ultimate goal is, of course, the interpretation of observed solar wind phenomena as the effects of basic physical processes occurring in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "large-scale" features revealed by the observations. It requires extensive use of the concepts and methods of fluid mechanics Physics Physical geography Meteorology Astronomy, Observations and Techniques Astrophysics and Astroparticles Meteorology/Climatology Geophysics/Geodesy Sonnenwind (DE-588)4135572-6 gnd rswk-swf Expansion (DE-588)4247031-6 gnd rswk-swf Sonnenkorona (DE-588)4181832-5 gnd rswk-swf Sonnenkorona (DE-588)4181832-5 g Expansion (DE-588)4247031-6 s Sonnenwind (DE-588)4135572-6 s 1\p DE-604 https://doi.org/10.1007/978-3-642-65414-5 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Hundhausen, A. J. Coronal Expansion and Solar Wind Physics Physical geography Meteorology Astronomy, Observations and Techniques Astrophysics and Astroparticles Meteorology/Climatology Geophysics/Geodesy Sonnenwind (DE-588)4135572-6 gnd Expansion (DE-588)4247031-6 gnd |
| subject_GND | (DE-588)4135572-6 (DE-588)4247031-6 (DE-588)4181832-5 |
| title | Coronal Expansion and Solar Wind |
| title_auth | Coronal Expansion and Solar Wind |
| title_exact_search | Coronal Expansion and Solar Wind |
| title_full | Coronal Expansion and Solar Wind by A. J. Hundhausen |
| title_fullStr | Coronal Expansion and Solar Wind by A. J. Hundhausen |
| title_full_unstemmed | Coronal Expansion and Solar Wind by A. J. Hundhausen |
| title_short | Coronal Expansion and Solar Wind |
| title_sort | coronal expansion and solar wind |
| topic | Physics Physical geography Meteorology Astronomy, Observations and Techniques Astrophysics and Astroparticles Meteorology/Climatology Geophysics/Geodesy Sonnenwind (DE-588)4135572-6 gnd Expansion (DE-588)4247031-6 gnd |
| topic_facet | Physics Physical geography Meteorology Astronomy, Observations and Techniques Astrophysics and Astroparticles Meteorology/Climatology Geophysics/Geodesy Sonnenwind Expansion Sonnenkorona |
| url | https://doi.org/10.1007/978-3-642-65414-5 |
| work_keys_str_mv | AT hundhausenaj coronalexpansionandsolarwind |