Numerical 3D constraints on convective eddy time-correlations: Consequences for stochastic excitation of solar p modes

Astronomy and Astrophysics

Volumn 404, Issue 3, 2003, Pages 1129-1137

  Samadi, R ^a,b   Nordlund, A ^c   Stein, R F ^d   Goupil, M J ^b   Roxburgh, I ^a,b  

^a QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

^d MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

Convection; Stars: oscillations; Sun: oscillations; Turbulence

Indexed keywords

ACOUSTICS; COMPUTER SIMULATION; CORRELATION METHODS; ENTROPY; FOURIER TRANSFORMS; HEAT CONVECTION; OSCILLATIONS; RANDOM PROCESSES; STRESSES; TURBULENCE; VELOCITY;

STOCHASTIC EXCITATIONS;

SUN;

EID: 0038680599     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030504     Document Type: Article

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