Some peculiarities of the power spectrum of the 5-min solar brightness oscillations

Details Some peculiarities of the power spectrum of the 5-min solar brightness oscillations Some peculiarities of the power spectrum of the 5-min solar brightness oscillations

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..133...89b&link_type=abstract

(IRIS /International Research on the Interior of the Sun/ Workshop, 2nd, Tashkent, Uzbek SSR, Sept. 1989, Proceedings. A91-37551

Astronomy and Astrophysics

Astronomy

Power Spectra, Solar Flux, Solar Oscillations, Astronomical Photometry, Photometers, Spaceborne Astronomy, Temporal Distribution

Scientific paper

Several results of the solar irradiance observations carried out with the IPHIR experiment on board the Soviet spacecraft within the PHOBOS Project are considered. The time variations of the power spectrum of 5-min solar oscillations is discussed. It is found that the lines are generated inhomogeneously in the spectrum as a whole. Each of the frequencies is excited separately at a definite time interval. The duration of active periods does not exceed 2 or 3 hours.

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