Detection and classication of resolved multiplet members of the solar 5 minute oscillations through solar diameter-type observations

Details Detection and classication of resolved multiplet members of the solar 5 minute oscillations through solar diameter-type observations Detection and classication of resolved multiplet members of the solar 5 minute oscillations through solar diameter-type observations

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...290..765h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 290, March 15, 1985, p. 765-781. NSF-USAF-supported research.

Other

28

Fine Structure, Solar Oscillations, Solar Rotation, Doppler Effect, Energy Dissipation, Fraunhofer Lines, Power Spectra, Spectral Line Width, Zeeman Effect

Scientific paper

After Hill and Stebbins (1975) provided the first evidence of global oscillations in solar diameter observations, numerous attempts have been made to obtain similar evidence of these modes of oscillation in other types of observations, taking into account Doppler shifts of Fraunhofer lines. Unfortunately, efforts to detect the considered global solar oscillations by other types of observations have so far not been successful. The relative utility of the observational techniques currently in use could be evaluated on the basis of a direct comparison of various results regarding the five minute oscillations. New information obtained on five minute oscillations provides confirmation of the existence and detection of resolved members of multiplets through observed symmetry properties of the eigenfunctions. It is pointed out that the existence of such resolved multiplets is a pivotal issue at this time. The importance of this point is related to the implications for the internal rotation of the sun.

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