Magnetohydrodynamics of the Sun:
Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magn...
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2014
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| Subjects: | |
| Online Access: | DE-12 DE-92 Volltext |
| Summary: | Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at www.cambridge.org/9780521854719 |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xix, 560 pages) |
| ISBN: | 9781139020732 |
| DOI: | 10.1017/CBO9781139020732 |
Staff View
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| 505 | 8 | |a A description of the Sun -- Basic equations of MHD -- Magnetohydrostatics -- Waves -- Shock waves -- Magnetic reconnection -- Instability -- Dynamo theory -- Magnetoconvection and sunspots -- Heating of the upper atmosphere -- Prominences -- Solar flares and coronal mass ejections -- The solar wind -- Appendices | |
| 520 | |a Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at www.cambridge.org/9780521854719 | ||
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Record in the Search Index
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| author | Priest, E. R. 1943- |
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| contents | A description of the Sun -- Basic equations of MHD -- Magnetohydrostatics -- Waves -- Shock waves -- Magnetic reconnection -- Instability -- Dynamo theory -- Magnetoconvection and sunspots -- Heating of the upper atmosphere -- Prominences -- Solar flares and coronal mass ejections -- The solar wind -- Appendices |
| ctrlnum | (ZDB-20-CBO)CR9781139020732 (OCoLC)907963497 (DE-599)BVBBV043944017 |
| dewey-full | 523.7/2 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.7/2 |
| dewey-search | 523.7/2 |
| dewey-sort | 3523.7 12 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9781139020732 |
| format | Electronic eBook |
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| isbn | 9781139020732 |
| language | English |
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| spelling | Priest, E. R. 1943- Verfasser aut Magnetohydrodynamics of the Sun Eric Priest, University of St. Andrews Cambridge Cambridge University Press 2014 1 online resource (xix, 560 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) A description of the Sun -- Basic equations of MHD -- Magnetohydrostatics -- Waves -- Shock waves -- Magnetic reconnection -- Instability -- Dynamo theory -- Magnetoconvection and sunspots -- Heating of the upper atmosphere -- Prominences -- Solar flares and coronal mass ejections -- The solar wind -- Appendices Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at www.cambridge.org/9780521854719 Solar activity Magnetohydrodynamics Solar magnetic fields Astrophysics Magnetohydrodynamik (DE-588)4130803-7 gnd rswk-swf Sun Sonne (DE-588)1236963652 gnd rswk-swf Magnetohydrodynamik (DE-588)4130803-7 s Sonne (DE-588)1236963652 g 1\p DE-604 Erscheint auch als Druckausgabe 978-0-521-85471-9 https://doi.org/10.1017/CBO9781139020732 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Priest, E. R. 1943- Magnetohydrodynamics of the Sun A description of the Sun -- Basic equations of MHD -- Magnetohydrostatics -- Waves -- Shock waves -- Magnetic reconnection -- Instability -- Dynamo theory -- Magnetoconvection and sunspots -- Heating of the upper atmosphere -- Prominences -- Solar flares and coronal mass ejections -- The solar wind -- Appendices Solar activity Magnetohydrodynamics Solar magnetic fields Astrophysics Magnetohydrodynamik (DE-588)4130803-7 gnd |
| subject_GND | (DE-588)4130803-7 (DE-588)1236963652 |
| title | Magnetohydrodynamics of the Sun |
| title_auth | Magnetohydrodynamics of the Sun |
| title_exact_search | Magnetohydrodynamics of the Sun |
| title_full | Magnetohydrodynamics of the Sun Eric Priest, University of St. Andrews |
| title_fullStr | Magnetohydrodynamics of the Sun Eric Priest, University of St. Andrews |
| title_full_unstemmed | Magnetohydrodynamics of the Sun Eric Priest, University of St. Andrews |
| title_short | Magnetohydrodynamics of the Sun |
| title_sort | magnetohydrodynamics of the sun |
| topic | Solar activity Magnetohydrodynamics Solar magnetic fields Astrophysics Magnetohydrodynamik (DE-588)4130803-7 gnd |
| topic_facet | Solar activity Magnetohydrodynamics Solar magnetic fields Astrophysics Magnetohydrodynamik Sun Sonne |
| url | https://doi.org/10.1017/CBO9781139020732 |
| work_keys_str_mv | AT priester magnetohydrodynamicsofthesun |