Cosmic Plasma Physics:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
2000
|
| Schriftenreihe: | Astrophysics and Space Science Library
251 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | of the approximation at hand will be outlined from the viewpoint of physics rather than of many possible astronomical applications. After that, as an aid to detailed understanding, please return with pencil and paper to work out the missing steps (if any) in the formal mathematics. On the basis of such an approach the student interested in modern astrophysics, its current practice, will find the answers to two key questions: (1) what approximation is the best one (the simplest but sufficient) for description of a phenomenon in cosmic plasma; (2) how to build an adequate model for the phenomenon, for example, a solar flare. Practice is really important for understanding the theory of cosmic plasma. Related exercises (problems and answers supplemented to each chapter) to improve skill do not thwart the theory but serve to better understanding of cosmic plasma physics. As for the applications, preference evidently is given to physical processes in the solar plasma. Why? - Much attention to solar plasma physics is conditioned by the possibility of the all-round observational test of theoretical models. This statement primarily relates to the processes in the solar atmosphere. For instance, flares on the Sun, in contrast to those on other stars as well as a lot of other analogous phenomena in the Universe, can be seen in their development, i. e |
| Beschreibung: | 1 Online-Ressource (XX, 652 p) |
| ISBN: | 9789401595926 9789048155385 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-015-9592-6 |
Internformat
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Datensatz im Suchindex
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| id | DE-604.BV042416211 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:59Z |
| institution | BVB |
| isbn | 9789401595926 9789048155385 |
| issn | 0067-0057 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027851704 |
| oclc_num | 863942827 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (XX, 652 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 2000 |
| publishDateSearch | 2000 |
| publishDateSort | 2000 |
| publisher | Springer Netherlands |
| record_format | marc |
| series | Astrophysics and Space Science Library |
| series2 | Astrophysics and Space Science Library |
| spelling | Somov, Boris V. Verfasser aut Cosmic Plasma Physics by Boris V. Somov Dordrecht Springer Netherlands 2000 1 Online-Ressource (XX, 652 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library 251 0067-0057 of the approximation at hand will be outlined from the viewpoint of physics rather than of many possible astronomical applications. After that, as an aid to detailed understanding, please return with pencil and paper to work out the missing steps (if any) in the formal mathematics. On the basis of such an approach the student interested in modern astrophysics, its current practice, will find the answers to two key questions: (1) what approximation is the best one (the simplest but sufficient) for description of a phenomenon in cosmic plasma; (2) how to build an adequate model for the phenomenon, for example, a solar flare. Practice is really important for understanding the theory of cosmic plasma. Related exercises (problems and answers supplemented to each chapter) to improve skill do not thwart the theory but serve to better understanding of cosmic plasma physics. As for the applications, preference evidently is given to physical processes in the solar plasma. Why? - Much attention to solar plasma physics is conditioned by the possibility of the all-round observational test of theoretical models. This statement primarily relates to the processes in the solar atmosphere. For instance, flares on the Sun, in contrast to those on other stars as well as a lot of other analogous phenomena in the Universe, can be seen in their development, i. e Physics Nuclear physics Theoretical, Mathematical and Computational Physics Nuclear Physics, Heavy Ions, Hadrons Astrophysics and Astroparticles Astrophysics and Space Science Library 251 (DE-604)BV000000296 251 https://doi.org/10.1007/978-94-015-9592-6 Verlag Volltext |
| spellingShingle | Somov, Boris V. Cosmic Plasma Physics Astrophysics and Space Science Library Physics Nuclear physics Theoretical, Mathematical and Computational Physics Nuclear Physics, Heavy Ions, Hadrons Astrophysics and Astroparticles |
| title | Cosmic Plasma Physics |
| title_auth | Cosmic Plasma Physics |
| title_exact_search | Cosmic Plasma Physics |
| title_full | Cosmic Plasma Physics by Boris V. Somov |
| title_fullStr | Cosmic Plasma Physics by Boris V. Somov |
| title_full_unstemmed | Cosmic Plasma Physics by Boris V. Somov |
| title_short | Cosmic Plasma Physics |
| title_sort | cosmic plasma physics |
| topic | Physics Nuclear physics Theoretical, Mathematical and Computational Physics Nuclear Physics, Heavy Ions, Hadrons Astrophysics and Astroparticles |
| topic_facet | Physics Nuclear physics Theoretical, Mathematical and Computational Physics Nuclear Physics, Heavy Ions, Hadrons Astrophysics and Astroparticles |
| url | https://doi.org/10.1007/978-94-015-9592-6 |
| volume_link | (DE-604)BV000000296 |
| work_keys_str_mv | AT somovborisv cosmicplasmaphysics |