Physics
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981vsc..conf..131c&link_type=abstract
In its Variations of the Solar Constant p 131-136 (SEE N82-17014 07-92)
Physics
2
Luminosity, Matching, Perturbation, Prediction Analysis Techniques, Solar Constant, Solar Flux Density, Variations, Estimating, Illuminance, Mathematical Models, Particle Flux Density, Radiant Flux Density, Solar Physics
Scientific paper
A simple matching technique is explained which allows the computation of the response of the solar surface to perturbations which occur at any depth within the convective envelope of the Sun. This technique was applied to a perturbation of the convective efficiency (alpha-mechanism), and of the non-gas component of the pressure (beta-mechanism) in different regions of the convection zone. The results indicate that either perturbation affects the solar luminosity. However, the alpha-mechanism has little effect in the solar radius, regardless of the location of the perturbed region, whereas the beta-mechanism produces radius changes that become quite large if the location of the perturbed region is deep within the solar convection zone.
Chan Kwan-Leung
Sofia Sabatino
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