Modeling the excitation of acoustic modes in α Centauri A

Astronomy and Astrophysics

Volumn 489, Issue 1, 2008, Pages 291-299

  Samadi, R ^a   Belkacem, K ^a   Goupil, M J ^a   Dupret, M A ^a   Kupka, F ^b  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Convection; Stars: atmospheres; Stars: oscillations; Turbulence

Indexed keywords

ACOUSTICS; ERROR ANALYSIS; NANOTECHNOLOGY; REYNOLDS NUMBER; SEISMOLOGY; SOLAR ENERGY; SUN; TURBULENCE;

ACOUSTIC MODES; CONVECTION; ENTROPY FLUCTUATIONS; ERROR BARS; EXCITATION RATES; GAUSSIAN; HELIOSEISMIC DATA; LORENTZIAN; MODE EXCITATION; OBSERVATIONAL DATA; QUASI-NORMAL APPROXIMATION; REYNOLDS STRESSES; SEISMIC MEASUREMENTS; STARS: ATMOSPHERES; STARS: OSCILLATIONS; TIME CORRELATION FUNCTION; TIME CORRELATIONS; TURBULENT CONVECTION; TURBULENT PRESSURE; TWO SOURCES;

CORRELATION METHODS;

EID: 52649088873     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078738     Document Type: Article

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