Low-l p-mode solar eigenfrequency measurements from the Birmingham Network

Details Low-l p-mode solar eigenfrequency measurements from the Birmingham Network Low-l p-mode solar eigenfrequency measurements from the Birmingham Network

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251p...7e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, July 1, 1991, p. 7P-9P. Research supported by SERC

Astronomy and Astrophysics

Astronomy

25

Acoustic Frequencies, Helioseismology, P Waves, Solar Oscillations, Solar Cycles, Solar Interior, Stellar Models

Scientific paper

Observations of the acoustic oscillations of the sun taken over a period of eight years are presented and discussed in terms of their implications regarding the nature of the deep solar interior. Stable atomic standards are used to integrate light from the whole solar disc, and the data taken over the course of the measurements are averaged to examine the mean frequencies for all the modes. The quality of the data allows comparisons with solar theories as well as the analysis of long-term solar cycle trends.

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