Detection of 160-min solar oscillations and atmospheric extinction

Details Detection of 160-min solar oscillations and atmospheric extinction Detection of 160-min solar oscillations and atmospheric extinction

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..317s&link_type=abstract

Astronomy and Astrophysics, vol. 88, no. 3, Aug. 1980, p. 317-319.

Astronomy and Astrophysics

Astrophysics

5

Atmospheric Attenuation, Earth Atmosphere, Solar Oscillations, Solar Terrestrial Interactions, Magnetic Signatures, Solar Rotation, Statistical Analysis

Scientific paper

The influence of the earth's atmosphere on the search for global solar oscillations with a period of 160m is studied. It is shown that neither the amplitude nor the phase behavior of the oscillations persisting during the last five years (1974-1978) can be explained in terms of the terrestrial atmospheric influences or by the statistical method of treatment. The observational evidence strongly suggests that the 160m periodicity is of solar origin.

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