Analysis of MDI high-degree solar-p mode parameters

Details Analysis of MDI high-degree solar-p mode parameters Analysis of MDI high-degree solar-p mode parameters

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp21a..03r&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP21A-03

Physics

7522 Helioseismology, 7536 Solar Activity Cycle (2162)

Scientific paper

We present a detailed analysis of solar acoustic mode parameters for modes with degree up to 900. They were obtained by applying spherical harmonic decomposition to full-disk solar images observed by the Michelson Doppler Imager (MDI) on board the Solar and Heliospheric Observatory (SOHO) spacecraft. We have analyzed seven observational periods (2-3 months long) from 1999 to 2005. A physically motivated model including a complete leakage matrix was used to recover the actual high-degree mode characteristics.

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