Seismology of the Sun and the Distant Stars:
Gespeichert in:
| Weitere Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1986
|
| Schriftenreihe: | NATO ASI Series, C: Mathematical and Physical Sciences
169 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The history of modern helioseismology is only ten years old. In 1975 F-L Deubner separated for the first time the spatial and temporal properties of the solar five-minute oscillations, and was thus able to measure the dispersion relation for high-degree acoustic modes (p modes). The diagnostic value of these observations was appreciated immediately. Indeed, by comparing the observed relation with computations that had already been carried out by R.K. Ulrich, and subsequently by H. Ando and Y. Osaki, it was recognised that contemporary solar models that had been constructed with the low observed neutrino flux in mind were too hot in their outer layers. Moreover, their convection zones were too shallow. Since that time the observations have improved. There is now good reason to suppose that a sufficiently careful analysis will lead to a direct determination of the helium abundance in the solar convection zone, especially when foreseeable further improvements in the observations have been achieved. The data will also provide useful diagnostics of the uncertain equation of state of partially ionized plasmas, and they might also enable us to measure the large-scale structure of the convective flow |
| Beschreibung: | 1 Online-Ressource (492p) |
| ISBN: | 9789400946088 9789401085472 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-009-4608-8 |
Internformat
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Datensatz im Suchindex
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| discipline | Physik |
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| spelling | Gough, Douglas O. 1941- (DE-588)104796340X edt Seismology of the Sun and the Distant Stars edited by D. O. Gough Proceedings of the NATO Advanced Research Workshop, Cambridge, U.K., June 17-21, 1985 Dordrecht Springer Netherlands 1986 1 Online-Ressource (492p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, C: Mathematical and Physical Sciences 169 1389-2185 The history of modern helioseismology is only ten years old. In 1975 F-L Deubner separated for the first time the spatial and temporal properties of the solar five-minute oscillations, and was thus able to measure the dispersion relation for high-degree acoustic modes (p modes). The diagnostic value of these observations was appreciated immediately. Indeed, by comparing the observed relation with computations that had already been carried out by R.K. Ulrich, and subsequently by H. Ando and Y. Osaki, it was recognised that contemporary solar models that had been constructed with the low observed neutrino flux in mind were too hot in their outer layers. Moreover, their convection zones were too shallow. Since that time the observations have improved. There is now good reason to suppose that a sufficiently careful analysis will lead to a direct determination of the helium abundance in the solar convection zone, especially when foreseeable further improvements in the observations have been achieved. The data will also provide useful diagnostics of the uncertain equation of state of partially ionized plasmas, and they might also enable us to measure the large-scale structure of the convective flow Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Stern (DE-588)4057342-4 gnd rswk-swf Seismologie (DE-588)4379341-1 gnd rswk-swf Sonne (DE-588)1236963652 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1985 Cambridge gnd-content Seismologie (DE-588)4379341-1 s Sonne (DE-588)1236963652 g 2\p DE-604 Stern (DE-588)4057342-4 s 3\p DE-604 NATO ASI Series, C Mathematical and Physical Sciences 169 (DE-604)BV000902768 169 https://doi.org/10.1007/978-94-009-4608-8 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Seismology of the Sun and the Distant Stars Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Stern (DE-588)4057342-4 gnd Seismologie (DE-588)4379341-1 gnd |
| subject_GND | (DE-588)4057342-4 (DE-588)4379341-1 (DE-588)1236963652 (DE-588)1071861417 |
| title | Seismology of the Sun and the Distant Stars |
| title_alt | Proceedings of the NATO Advanced Research Workshop, Cambridge, U.K., June 17-21, 1985 |
| title_auth | Seismology of the Sun and the Distant Stars |
| title_exact_search | Seismology of the Sun and the Distant Stars |
| title_full | Seismology of the Sun and the Distant Stars edited by D. O. Gough |
| title_fullStr | Seismology of the Sun and the Distant Stars edited by D. O. Gough |
| title_full_unstemmed | Seismology of the Sun and the Distant Stars edited by D. O. Gough |
| title_short | Seismology of the Sun and the Distant Stars |
| title_sort | seismology of the sun and the distant stars |
| topic | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Stern (DE-588)4057342-4 gnd Seismologie (DE-588)4379341-1 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Stern Seismologie Sonne Konferenzschrift 1985 Cambridge |
| url | https://doi.org/10.1007/978-94-009-4608-8 |
| volume_link | (DE-604)BV000902768 |
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