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Interaction of convection and oscillations in the solar atmosphere: numerical results

Published online by Cambridge University Press:  03 August 2017

M. Steffen
M. Steffen*
Affiliation:
Institut für Theoretische Physik u. Sternwarte, Universität Kiel, Olshausenstraße 40, D-2300 KIEL 1, West Germany

Abstract

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Analysing the results of numerical simulations of solar granular convection we found, superimposed on the convective flow, an oscillatory phenomenon with a well defined period of 260 ± 15 sec.

Type
Chapter 6: Excitation and Damping of Solar and Stellar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 379 - 382
Copyright
Copyright © Reidel 1988 

References

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