Measurements of solar oscillations at 37 GHz

Details Measurements of solar oscillations at 37 GHz Measurements of solar oscillations at 37 GHz

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..235t&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 235-239 (SEE N89-25819 19-92)

Other

Extremely High Frequencies, Helioseismology, Solar Activity, Solar Oscillations, Amplitude Distribution Analysis, Data Acquisition, Power Spectra, Solar Spectra

Scientific paper

Observations at 37 GHz of solar oscillations made during August 1983 and May 1988 at Metsahovi (Finland) are presented. Altogether, data from 10 clear days could be used for further analysis. Five quiet regions were selected from the Sun and the amplitude differences were monitored during the day. Due to the large amount of data only typical examples are presented. During favorable conditions the amplitude at the period of 160 min increases in respect to the other peaks in the power spectrum. The data also suggest that a higher degree g-mode oscillation, (greater than or = 5) could be possible.

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