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High-Frequency Solar Oscillations

Published online by Cambridge University Press:  08 February 2017

Stuart M. Jefferies
Stuart M. Jefferies*
Affiliation:
National Solar Observatory, Tucson, AZ, USA

Abstract

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This paper reviews the properties of the solar oscillation power spectrum at frequencies near and above the acoustic cut-off frequency for the atmosphere. This region of the spectrum contains over 50% of the total peak structure observed and is a source of information not only on the outer layers of the sun and the origin of solar oscillations, but also on the physics of the solar core and chromosphere.

Type
VII. The Solar Atmosphere
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 415 - 422
Copyright
Copyright © Kluwer 1998 

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