Physics
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994alab.reptq....m&link_type=abstract
Final Report Alabama Univ., Huntsville, AL. Dept. of Mechanical and Aerospace Engineering.
Physics
Acoustic Propagation, Chromosphere, Convective Heat Transfer, Coronal Holes, Flux Transfer Events, Solar Atmosphere, Solar Wind, Turbulence, Turbulent Flow, Wave Generation, Coupling, Dwarf Stars, Spectral Emission, Stellar Coronas
Scientific paper
New calculations of the acoustic wave energy fluxes generated in the solar convective zone have been performed. The treatment of convective turbulence in the sun and solar-like stars, in particular, the precise nature of the turbulent power spectrum has been recognized as one of the most important issues in the wave generation problem. Several different functional forms for spatial and temporal spectra have been considered in the literature and differences between the energy fluxes obtained for different forms often exceed two orders of magnitude. The basic criterion for choosing the appropriate spectrum was the maximal efficiency of the wave generation. We have used a different approach based on physical and empirical arguments as well as on some results from numerical simulation of turbulent convection.
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