Probing the solar core with BiSON: the challenge at low l and low frequency

Details Probing the solar core with BiSON: the challenge at low l and low frequency Probing the solar core with BiSON: the challenge at low l and low frequency

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..183c&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Physics

Sun: Interior, Sun: Oscillations

Scientific paper

In this contribution we touch upon a few issues of relevance to the current status of low-angular-degree (low-l) p-mode Helioseismology. In particular: the precision in frequency, both historic and current, achievable at low l; the quest to extend the low-frequency detection threshold nearer to the p-mode fundamental; and the level of agreement between frequencies extracted from different data using various analysis techniques.

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