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Source Depth for Solar p-Modes

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Published 2000 November 21 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Pawan Kumar and Sarbani Basu 2000 ApJ 545 L65 DOI 10.1086/317325

1538-4357/545/1/L65

Abstract

Theoretically calculated power spectra are comparable with observed solar p-mode velocity power spectra over a range of mode, degree, and frequency. The depth for the sources responsible for exciting p-modes of frequency 2.0 mHz is determined from the asymmetry of their power spectra and found to be about 800 km below the photosphere for quadrupole sources and 150 km if sources are dipole. The source depth for high-frequency oscillations greater than ~6 mHz is 180 (50) km for quadrupole (dipole) sources.

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10.1086/317325