Mode visibilities in radial velocity and intensity Sun-as-a-star helioseismic measurements
DOI: 10.1088/1742-6596/271/1/012053
Bibcode: 2011JPhCS.271a2053S
García, R. A.; Ballot, J.; Salabert, D.
Spain, France
Abstract
We analyze more than 5000 days of Sun-as-a-star radial velocity GOLF and intensity VIRGO observations to measure the visibilities of the I = 0, 1, 2, and 3 modes and the m-amplitude ratios of the I = 2 and 3 modes in the solar acoustic spectrum. We provide observational values that we compare to theoretical predictions.
2011
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GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO
1