SOHO 18/GONG 2006/HELAS I Beyond the spherical Sun

By J. Toomre, M. Thompson. 2006

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Automated extraction of oscillation parameters for Kepler observations of solar-type stars (2009, unknown): “For the analysis of red giants observed with CoRoT, Kallinger et al. (2009) used simultaneous fitting of the background and the oscillation power excess, with the latter modelled with a Gaussian function.”
Helioseismology and Solar Abundances (2007, background): “Basu & Antia (1997) found that the density profiles of solar envelope models constructed to have the correct convection-zone depth and helium abundance is extremely sensitive to the heavy-element abundance.”
FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY (2013, unknown): “Solar-like oscillations are acoustic standing waves excited by near-surface convection (see, e.g., Houdek et al. 1999; Houdek 2006; Samadi et al. 2007).”
NEW SOLAR COMPOSITION: THE PROBLEM WITH SOLAR MODELS REVISITED (2009, background): “26 68 v2 [ Subject headings: Sun: helioseismology - Sun: interior - Sun: abundances - neutrinos”
FUNDAMENTAL PROPERTIES OF STARS USING ASTEROSEISMOLOGY FROM KEPLER AND CoRoT AND INTERFEROMETRY FROM THE CHARA ARRAY (2012, background): “The launches of the space telescopes CoRoT (Convection, Rotation and planetary Transits, Baglin et al. 2006a,b) and Kepler (Borucki et al. 2010; Koch et al. 2010) has increased the number of stars with detected solar-like oscillations to several thousands, providing a large sample spanning from the ”