Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...74.1129l&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 74, Dec. 1990, p. 1129-1149.
Astronomy and Astrophysics
Astrophysics
183
Frequency Distribution, Harmonic Oscillation, Solar Oscillations, Spatial Distribution, Helioseismology, Power Spectra
Scientific paper
Solar oscillations have been observed at three different spatial scales at Big Bear Solar Observatory during 1986-1987 and, using three data sets, a new and more accurate table of solar oscillation frequencies has been compiled. The oscillations, which are presented as functions of radial order n and spherical harmonic degree l, are averages over azimuthal order and therefore approximate the normal mode frequencies of a nonrotating, spherically symmetric sun, near solar minimum. The table contains frequencies for most of the solar p and f modes with l between 0 and 1860, n between 0 and 26, and oscillation mode frequencies between 1.0 and 5.3.
Kaufman Michael J.
Libbrecht Kenneth G.
Woodard Martin F.
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