The nature of solar 160-min oscillations

Details The nature of solar 160-min oscillations The nature of solar 160-min oscillations

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..637r&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, July 1988, p. 637-643. In Russian. In Russian.

Computer Science

Numerical Analysis

Atmospheric Attenuation, Atmospheric Refraction, Earth Atmosphere, Solar Oscillations, Solar Rotation, Numerical Analysis, Radial Velocity

Scientific paper

The influence of the differential effects of refraction and absorption in the earth's atmosphere on solar radial velocity oscillations is considered. Of particular interest are spacing, duration, the seasonal effect on the observations, and methods for discerning a trend in the radial velocity signal. Arguments suggesting that these oscillations are solar in nature with P = 160 min are analyzed.

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