Seismic sun

Chitre, S. M. ; Antia, H. M. (1999) Seismic sun Current Science, 77 (11). pp. 1454-1460. ISSN 0011-3891

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Even though the interior of the sun is not directly accessible to observations, it is nonetheless possible to infer the physical conditions inside the sun using the theory of stellar structure and the accurately measured frequencies of solar oscillations. The heloiseismic data has provided a powerful tool to probe the sun and also to test physical theories describing its internal constitution.

Item Type:Article
Source:Copyright of this article belongs to Current Science Association.
ID Code:75617
Deposited On:24 Dec 2011 15:06
Last Modified:18 May 2016 19:34

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