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Variable Stars as Essential Astrophysical Tools pp 59–168Cite as

An Introduction to Helioseismology

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Part of the book series: NATO Science Series ((ASIC,volume 544))

Abstract

In no other case has stellar variability been honed to such a sharp astrophysical tool as for the Sun. The extreme richness of oscillation data available for the Sun, as a result of its proximity and the nature of the excitation processes responsible for the oscillations, provides us with a scalpel which allows us to dissect in minute detail, layer by layer, the physical properties of the solar interior.

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Authors and Affiliations

  1. Teoretisk Astrofysik Center, Danmarks Grundforskningsfond, and Institut for Fysik og Astronomy, Aarhus Universitet, Aarhus C, DK-8000, Denmark

    Jørgen Christensen-Dalsgaard

  2. Department of Physics and Astronomy, University of Southern California, Los Angeles, CA, 90089, USA

    Werner Däppen

  3. Teoretisk Astrofysik Center, Aarhus Universitet, Aarhus C, DK-8000, Denmark

    Werner Däppen

  4. Obserwatorium Astronomiczne, Uniwersytetu Warszawskiego, Al. Ujazdowskie 4, Warszawa, 00-478, Poland

    Woiciech A. Dziembowski

  5. Centrum Astronomiczne im., Mikołaja Kopernika, ul. Bartycka 18, Warszawa, 00-716, Poland

    Woiciech A. Dziembowski

  6. Applied Theoretical and Computational Physics Division, Los Alamos National Laboratory, XTA MS B220, Los Alamos, NM, 87545, USA

    Joyce A. Guzik

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  1. Jørgen Christensen-Dalsgaard
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  2. Werner Däppen
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  3. Woiciech A. Dziembowski
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  4. Joyce A. Guzik
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  1. Astronomy and Space Sciences Department, Ege University Science Faculty, Bornova, İzmir, Turkey

    Cafer İbanoğlu

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Christensen-Dalsgaard, J., Däppen, W., Dziembowski, W.A., Guzik, J.A. (2000). An Introduction to Helioseismology. In: İbanoğlu, C. (eds) Variable Stars as Essential Astrophysical Tools. NATO Science Series, vol 544. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4299-1_2

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