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Helio- and Asteroseismic Analysis Methods

Published online by Cambridge University Press:  30 March 2016

Jesper Schou
Jesper Schou*
Affiliation:
Stanford University, HEPL Annex A201, Stanford, CA 94305-4085, USA

Abstract

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Over the past couple of decades increasingly sophisticated analysis algorithms have been developed in helioseismology. Here I will describe some of these with an emphasis on those most relevant to asteroseismology and some of the lessons learned. I will also discuss some of the properties of stellar oscillations and how those affect the analysis.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 415 - 418
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Anderson, E. R., Duvall, T. L. Jr. & Jefferies, S. M. 1990, ApJ, 364, 699 Google Scholar
Appourchaux, T. 2003, Ap&SS, 284, 109 Google Scholar
Basu, S., et al. 2003, ApJ, 591, 432 Google Scholar
Bouchy, F. & Carrier, F. 2002, A&A, 390, 205 Google Scholar
Hill, F., et al. 1996, Science, 272, 1292 Google Scholar
Korzennik, S. G., Rabello-Soares, M. C. & Schou, J. 2003, ApJ, 602, 481 (stro-ph/0207371)Google Scholar
Rhodes, E. J. Jr, et al. 2001, ApJ, 561, 1127 Google Scholar
Schou, J. 1992, PhD Dissertation, University of Aarhus, Denmark Google Scholar
Schou, J. 1998, SOHO 6/GONG 98, ESA SP-418, 47 Google Scholar
Schou, J. & Buzasi, D. L. 2001, SOHO 10/GONG 2000, ESA SP-464, 391 Google Scholar
Schou, J., et al. 2002, ApJ, 567, 1234 Google Scholar