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A New Class of Solar Oscillation Measurements

Published online by Cambridge University Press:  13 May 2016

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

Abstract

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Over the past few years the quality and quantity of basic helioseismic data have increased dramatically as instruments such as MDI on the SOHO spacecraft and the GONG network have become operational. The data from these new instruments have led to a significant increase in our ability to make inferences about the solar interior, and resulted in a long series of often surprising and spectacular discoveries. In this review I describe some of the most recent results and what progress we may be able to make in the near future with improved analysis methods and with a better understanding of solar oscillations and the instruments used to observe them.

Type
Session I: Global Structure and Evolution of the Solar Interior
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 21 - 28
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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