Advances in helioseismology

Details Advances in helioseismology Advances in helioseismology

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sci...253..152l&link_type=abstract

Science (ISSN 0036-8075), vol. 253, July 12, 1991, p. 152-157.

Computer Science

79

Helioseismology, Solar Interior, Solar Rotation, Stellar Oscillations, Line Spectra, Time Dependence

Scientific paper

The paper discusses the characteristics of recently-discovered oscillation modes in the sun that are phase-coherent for up to 1 yr, with surface velocity amplitudes as low as 2 mm/sec. Particular attention is given to the properties of p-modes and f-modes of the small-amplitude oscillations, for which there is clear and abundant observational data. Some properties of the solar interior are inferred from the comparison of p-mode frequencies with solar model calculations.

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