Solving the forward problem of helioseismology in the frequency domain
International audienceSolar acoustic waves are continuously excited by turbulent convection (a random process). The forward problem of local helioseismology was specified at the Waves 2013 conference: computing the cross-covariance of the wave field ...
Gizon, Laurent +6 more
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Chandrasekhar's Conditions for the Equilibrium and Stability of Stars in a Universal Three-Parameter Non-Maxwell Distribution. [PDF]
Hu W, Du J.
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Weak influence of near-surface layer on solar deep convection zone revealed by comprehensive simulation from base to surface. [PDF]
Hotta H, Iijima H, Kusano K.
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A new method for detecting solar atmospheric gravity waves. [PDF]
Calchetti D +4 more
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Subgiants in NGC 188 reveal that rotationally induced mixing creates the main sequence Li-Dip. [PDF]
Sun Q +6 more
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VALIDATING FORWARD MODELING AND INVERSIONS OF HELIOSEISMIC HOLOGRAPHY MEASUREMENTS. [PDF]
DeGrave K +4 more
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Inference of dominant modes for linear stochastic processes. [PDF]
MacKay RS.
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Flows around Averaged Solar Active Regions. [PDF]
Braun DC.
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Solar system expansion and strong equivalence principle as seen by the NASA MESSENGER mission. [PDF]
Genova A +6 more
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