Effect of Turbulent Pressure on Solar Oscillation Frequencies View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1997

AUTHORS

H. M. Antia , Sarbani Basu

ABSTRACT

We use observed frequencies of solar p-modes to test different formulations for calculating the convective flux. In particular, models using the usual mixing length theory and the formulation of Canuto and Mazzitelli for calculating the convective flux are compared to find that the latter yields frequencies that are closer to observed values. Inclusion of turbulent pressure is also found to improve the agreement with observed frequencies, but the magnitude of the difference is much smaller. More... »

PAGES

51-54

Book

TITLE

SCORe ’96: Solar Convection and Oscillations and their Relationship

ISBN

978-94-010-6172-8
978-94-011-5167-2

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-011-5167-2_3

DOI

http://dx.doi.org/10.1007/978-94-011-5167-2_3

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1015072863


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