Observations of solar oscillations with periods of 160 minutes

Details Observations of solar oscillations with periods of 160 minutes Observations of solar oscillations with periods of 160 minutes

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.277..635s&link_type=abstract

Nature, vol. 277, Feb. 22, 1979, p. 635-637.

Physics

30

Solar Atmosphere, Solar Oscillations, Graphs (Charts), Solar Physics

Scientific paper

Severny et al. (1976) have reported oscillations of the sun with a period near 160 min. A description is presented of observations made at the Stanford Solar Observatory during the time from 1975 to the present which seem to support the reports by Severny et al. At Stanford the relative velocity between a central circular area of radius 0.5 solar radius on the solar disk and most of the remaining area of the solar disk is measured. A superposed epoch analysis of the observations using a period of 160 min is discussed. An apparent agreement in phase between the obtained observational data and those reported by Severny et al. tends to support the interpretation that solar oscillations are being observed.

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