Statistical theory of turbulent convection in pulsating variables

Details Statistical theory of turbulent convection in pulsating variables Statistical theory of turbulent convection in pulsating variables

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977acasn..18...86x&link_type=abstract

Acta Astronomica Sinica, vol. 18, June 1977, p. 86-104. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

19

Atmospheric Turbulence, Convective Flow, Oscillating Flow, Statistical Analysis, Stellar Atmospheres, Variable Stars, Energy Transfer, Light Emission, Red Giant Stars, Steady Flow, Stellar Models, Stellar Radiation, Supergiant Stars, Viscous Flow

Scientific paper

The dynamic behavior of turbulent convection is statistically analyzed for both steady and pulsational components. The effects of viscosity and energy transfer on the oscillational stability of the convection are investigated. It is pointed out that these effects might account for the pulsational instability strip and the light variability of red giant and supergiant stars.

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