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http://hdl.handle.net/2248/1800
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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Dziembowski, W. A | - |
dc.date.accessioned | 2007-09-17T11:51:13Z | - |
dc.date.available | 2007-09-17T11:51:13Z | - |
dc.date.issued | 1996 | - |
dc.identifier.citation | BASI, Vol. 24, No. 2, pp. 133-142 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1800 | - |
dc.description.abstract | Only a small fraction of the solar p-modes have frequencies with any measurable sensitivity to the core structure. Nevertheless an accurate seismic sounding with such modes alone is possible. This requires a high-precision measurement of mode frequencies and a proper method of inversion. The important aspects here are elimination of the uncertainties concerning the outermost layers and making best use of a priori information about structural variables. Current data allow us to achieve an accuracy in pressure and density determination at the level of 1 percent in the bulk of the core. Results of helioseismic inversions support the standard picture of solar evolution. | en |
dc.format.extent | 943716 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1996BASI...24..133D | en |
dc.subject | Sun | en |
dc.subject | Interior - Sun | en |
dc.subject | Oscillations | en |
dc.title | Seismic probing of the solar core | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
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