Thermal perturbation of the Sun

Details Thermal perturbation of the Sun Thermal perturbation of the Sun

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981vsc..conf..137t&link_type=abstract

In NASA. Goddard Space Flight Center Variations of the Solar Constant p 137-142 (SEE N82-17014 07-92)

Physics

3

Convection, Luminosity, Mathematical Models, Perturbation, Solar Constant, Solar Diameter, Magnetic Disturbances, Solar Activity, Solar Physics, Variations

Scientific paper

An investigation of thermal perturbations of the solar convective zone via changes in the mixing length parameter were carried out, with a view toward understanding the possible solar radius and luminosity changes cited in the literature. The results show that: (a) a single perturbation of alpha is probably not the cause of the solar radius change and (b) the parameter W = d lambda nR./d lambda nL. can not be characterized by a single value, as implied in recent work.

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