Stochastic excitation of nonradial modes II. Are solar asymptotic gravity modes detectable?

Astronomy and Astrophysics

Volumn 494, Issue 1, 2009, Pages 191-204

  Belkacem, K ^a   Samadi, R ^a   Goupil, M J ^a   Dupret, M A ^a   Brun, A S ^b,c   Baudin, F ^d  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b CEA SACLAY   (France)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d UNIVERSITÉ PARIS SUD   (France)

Author keywords

Convection; Sun: oscillations; Turbulence

Indexed keywords

ASYMPTOTIC ANALYSIS; DAMPING; EXTRACTIVE METALLURGY; GRAVITATION; MOTION ESTIMATION; RANDOM PROCESSES; SOLAR ENERGY; THREE DIMENSIONAL; TURBULENCE; TURBULENT FLOW; VELOCITY;

3-D NUMERICAL SIMULATIONS; CONVECTION; CONVECTIVE VELOCITIES; CONVECTIVE ZONES; DAMPING RATES; FREQUENCY RANGES; G-MODES; GAUSSIAN; GLOBAL SIMULATIONS; GRAVITY MODES; LIFE-TIME; MAXIMUM VELOCITIES; MODE VELOCITIES; NON LOCALS; ORDERS OF MAGNITUDES; PARAMETRIC DESCRIPTIONS; RADIATIVE LOSS; SOLAR G MODES; STOCHASTIC EXCITATIONS; SUN: OSCILLATIONS; SURFACE VELOCITIES; THEORETICAL ESTIMATIONS; TIME DEPENDENTS; TURBULENT CONVECTIONS; TURBULENT EDDIES; TURBULENT ENERGY SPECTRUMS; UPPER LIMITS;

GRAVITATIONAL EFFECTS;

EID: 59449109186     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810827     Document Type: Article

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