Properties of intermediate-degree solar oscillation modes

Details Properties of intermediate-degree solar oscillation modes Properties of intermediate-degree solar oscillation modes

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..413l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 1, 1986, p. 413-423.

Computer Science

Sound

43

Helioseismology, Solar Oscillations, Eigenvalues, Sound Waves, Spherical Harmonics

Scientific paper

During the summer of 1985, 8042 high-resolution full disk Doppler images
of the Sun were obtained at Big Bear Solar Observatory in a 12 day
period. These images were analyzed for solar oscillation modes with
spherical harmonic degrees 5 ≤ l ≤ 20. The frequencies, lifetimes,
and amplitudes of these modes are presented.

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