The solar tachocline:
Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar interior. The unexpected discovery of an abrupt transition - the tachocline - between the differentially rotating convection zone and the uniformly rotating radiativ...
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| Weitere beteiligte Personen: | , , |
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| Format: | E-Book |
| Sprache: | Englisch |
| Veröffentlicht: |
Cambridge
Cambridge University Press
2007
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| Links: | https://doi.org/10.1017/CBO9780511536243 |
| Zusammenfassung: | Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar interior. The unexpected discovery of an abrupt transition - the tachocline - between the differentially rotating convection zone and the uniformly rotating radiative interior has generated considerable interest and raised many fundamental issues. This volume contains invited reviews from distinguished speakers at the first meeting devoted to the tachocline, held at the Isaac Newton Institute. It provides a comprehensive account of the understanding of the properties and dynamics of the tachocline, including both observational results and major theoretical issues, involving both hydrodynamic and magnetohydrodynamic behaviour. The Solar Tachocline is a valuable reference for researchers and graduate students in astrophysics, heliospheric physics and geophysics, and the dynamics of fluids and plasmas. |
| Umfang: | 1 Online-Ressource (xi, 367 Seiten) |
| ISBN: | 9780511536243 |
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| spelling | The solar tachocline edited by David W. Hughes, Robert Rosner, Nigel O. Weiss Cambridge Cambridge University Press 2007 1 Online-Ressource (xi, 367 Seiten) txt c cr Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar interior. The unexpected discovery of an abrupt transition - the tachocline - between the differentially rotating convection zone and the uniformly rotating radiative interior has generated considerable interest and raised many fundamental issues. This volume contains invited reviews from distinguished speakers at the first meeting devoted to the tachocline, held at the Isaac Newton Institute. It provides a comprehensive account of the understanding of the properties and dynamics of the tachocline, including both observational results and major theoretical issues, involving both hydrodynamic and magnetohydrodynamic behaviour. The Solar Tachocline is a valuable reference for researchers and graduate students in astrophysics, heliospheric physics and geophysics, and the dynamics of fluids and plasmas. Hughes, David W. 1941- Rosner, Robert Weiss, N. O. Erscheint auch als Druck-Ausgabe 9780521861014 Erscheint auch als Druck-Ausgabe 9781107405356 |
| spellingShingle | The solar tachocline |
| title | The solar tachocline |
| title_auth | The solar tachocline |
| title_exact_search | The solar tachocline |
| title_full | The solar tachocline edited by David W. Hughes, Robert Rosner, Nigel O. Weiss |
| title_fullStr | The solar tachocline edited by David W. Hughes, Robert Rosner, Nigel O. Weiss |
| title_full_unstemmed | The solar tachocline edited by David W. Hughes, Robert Rosner, Nigel O. Weiss |
| title_short | The solar tachocline |
| title_sort | solar tachocline |
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