Interpretations of the 160-minute solar oscillation

Details Interpretations of the 160-minute solar oscillation Interpretations of the 160-minute solar oscillation

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..238k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Mar. 1986, p. 238-246) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Mar.-Apr

Astronomy and Astrophysics

Astronomy

1

Solar Oscillations, Spectrum Analysis, Vibration Mode, Doppler Effect, Solar Rotation, Spatial Filtering, Spherical Harmonics

Scientific paper

Identification of solar oscillation with the 160-min period as a non-radial mode of the sun has been considered on the basis of the observational data recently available from several observatories. The amplitudes and phases observed allow the most probable identification of such an oscillation as a mode with degree l = 3 of a spherical harmonic. On the other hand however, the observed rotational splitting of the eigenfrequency due to solar rotation gives l = 1. New methods for future observations are considered to permit more reliable identification of the 160-min oscillations.

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