Changes Of The Solar Acoustic High-degree Mode Frequencies Over The Solar Cycle

Details Changes Of The Solar Acoustic High-degree Mode Frequencies Over The Solar Cycle Changes Of The Solar Acoustic High-degree Mode Frequencies Over The Solar Cycle

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0508k&link_type=abstract

American Astronomical Society, SPD meeting #37, #5.08; Bulletin of the American Astronomical Society, Vol. 38, p.224

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Using full-disk observations obtained with the Michelson Doppler Imager (MDI) on board the Solar and Heliospheric Observatory (SOHO) spacecraft, we present frequency and frequency splitting variations of high-degree (100 < l < 1000) solar acoustic modes over the solar cycle using global helioseismology analysis techniques. Since we analyzed high-degree modes, we focus on properties of the near-surface solar region. We have corrected for most of the known instrumental effects that affect the characterization of high-degree modes using the methodology described in Korzennik et al. (2004) as to estimate unbiased high-degree mode frequencies.

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