On model predictions of the power spectral density of radial solar p modes

Monthly Notices of the Royal Astronomical Society

Volumn 360, Issue 3, 2005, Pages 859-868

  Chaplin, W J ^a   Houdek, G ^b   Elsworth, Y ^a   Gough, D O ^b,c,d   Isaak, G R ^a   New, R ^e  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^e SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

Author keywords

Convection; Sun: helioseismology

Indexed keywords

REYNOLDS NUMBER; STOCHASTIC MODELS; STOCHASTIC SYSTEMS;

CONVECTION; FREQUENCIES DEPENDENCE; LOW DEGREE; MEASURED MODES; MODEL PREDICTION; POWER-SPECTRA; SOLAR P MODES; STOCHASTIC EXCITATION MODELS; SUN: HELIOSEISMOLOGY; TOTAL POWER;

POWER SPECTRAL DENSITY;

EID: 22144435184     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09041.x     Document Type: Article

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