Seismology of the sun and other stars

  • J. Christensen-Dalsgaard
Session II: Dynamos and Stellar Activity: Theory
Part of the Lecture Notes in Physics book series (LNP, volume 254)


Important results have already been obtained from helioseismology. As far as the solar structure is concerned, their most striking feature is perhaps how closely they agree with conventional solar models; this suggests that the solar neutrino problem may require a physical, rather than astrophysical, solution. However, the apparently complacent conclusion should not overshadow the fact that there remain substantial discrepancies, which are not understood, between the observed and computed oscillation frequencies. The inferred solar rotation curve is very far from expectations, and clearly raises important questions concerning the evolution of the solar internal rotation and the generation of the solar magnetic field. The observations now underway or being planned will contribute substantially to elucidating these problems.


Sound Speed Convection Zone Solar Magnetic Field Stellar Model Surface Rotation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer-Verlag 1986

Authors and Affiliations

  • J. Christensen-Dalsgaard
    • 1
  1. 1.Astronomisk InstitutAarhus UniversitetAarhus CDenmark

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