Physics of space plasma activity:
Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity event...
Gespeichert in:
1. Verfasser: | |
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Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Cambridge
Cambridge University Press
2007
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Schlagworte: | |
Online-Zugang: | BSB01 FHN01 Volltext |
Zusammenfassung: | Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity events observed in the solar system occur on the Sun, when coronal mass ejections expel several billion tons of plasma mass into space. This book provides a coherent and detailed treatment of the physical background of large plasma eruptions in space. It provides the background necessary for dealing with space plasma activity, and allows the reader to reach a deeper understanding of this fascinating natural event. The book employs both fluid and kinetic models, and discusses the applications to magnetospheric and solar activity. This will form an interesting reference for graduate students and academic researchers in the fields of astrophysics and plasma physics |
Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
Beschreibung: | 1 online resource (xxiii, 508 pages) |
ISBN: | 9780511618321 |
DOI: | 10.1017/CBO9780511618321 |
Internformat
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650 | 4 | |a Space plasmas | |
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Datensatz im Suchindex
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any_adam_object | |
author | Schindler, Karl 1931- |
author_GND | (DE-588)133296156 |
author_facet | Schindler, Karl 1931- |
author_role | aut |
author_sort | Schindler, Karl 1931- |
author_variant | k s ks |
building | Verbundindex |
bvnumber | BV043943440 |
classification_rvk | UR 8000 US 3500 US 6300 |
collection | ZDB-20-CBO |
ctrlnum | (ZDB-20-CBO)CR9780511618321 (OCoLC)699169524 (DE-599)BVBBV043943440 |
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 | 10.1017/CBO9780511618321 |
format | Electronic eBook |
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id | DE-604.BV043943440 |
illustrated | Not Illustrated |
indexdate | 2024-07-10T07:39:19Z |
institution | BVB |
isbn | 9780511618321 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029352411 |
oclc_num | 699169524 |
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owner | DE-12 DE-92 |
owner_facet | DE-12 DE-92 |
physical | 1 online resource (xxiii, 508 pages) |
psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
publishDate | 2007 |
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publishDateSort | 2007 |
publisher | Cambridge University Press |
record_format | marc |
spelling | Schindler, Karl 1931- Verfasser (DE-588)133296156 aut Physics of space plasma activity Karl Schindler Cambridge Cambridge University Press 2007 1 online resource (xxiii, 508 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity events observed in the solar system occur on the Sun, when coronal mass ejections expel several billion tons of plasma mass into space. This book provides a coherent and detailed treatment of the physical background of large plasma eruptions in space. It provides the background necessary for dealing with space plasma activity, and allows the reader to reach a deeper understanding of this fascinating natural event. The book employs both fluid and kinetic models, and discusses the applications to magnetospheric and solar activity. This will form an interesting reference for graduate students and academic researchers in the fields of astrophysics and plasma physics Space plasmas Astrophysik (DE-588)4003326-0 gnd rswk-swf Plasmaphysik (DE-588)4046259-6 gnd rswk-swf Astrophysik (DE-588)4003326-0 s Plasmaphysik (DE-588)4046259-6 s 1\p DE-604 Erscheint auch als Druckausgabe 978-0-521-14236-6 Erscheint auch als Druckausgabe 978-0-521-85897-7 https://doi.org/10.1017/CBO9780511618321 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
spellingShingle | Schindler, Karl 1931- Physics of space plasma activity Space plasmas Astrophysik (DE-588)4003326-0 gnd Plasmaphysik (DE-588)4046259-6 gnd |
subject_GND | (DE-588)4003326-0 (DE-588)4046259-6 |
title | Physics of space plasma activity |
title_auth | Physics of space plasma activity |
title_exact_search | Physics of space plasma activity |
title_full | Physics of space plasma activity Karl Schindler |
title_fullStr | Physics of space plasma activity Karl Schindler |
title_full_unstemmed | Physics of space plasma activity Karl Schindler |
title_short | Physics of space plasma activity |
title_sort | physics of space plasma activity |
topic | Space plasmas Astrophysik (DE-588)4003326-0 gnd Plasmaphysik (DE-588)4046259-6 gnd |
topic_facet | Space plasmas Astrophysik Plasmaphysik |
url | https://doi.org/10.1017/CBO9780511618321 |
work_keys_str_mv | AT schindlerkarl physicsofspaceplasmaactivity |