Identification of rotational modes in solar oscillations using radio observations.

Details Identification of rotational modes in solar oscillations using radio observations. Identification of rotational modes in solar oscillations using radio observations.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kpcb...12...14t&link_type=abstract

Kinematics Phys. Celest. Bodies, Vol. 12, No. 1, p. 14 - 19

Physics

Solar Oscillations: Solar Radio Radiation

Scientific paper

The author discusses the results of differential (limb-to-center) measurements of the quiet solar radio emission, made in 1978 - 1984. He shows that the interval 77 - 161 min contains combination periods from the interval 178 - 396 min. These periods are suggested to be periods of the synchronization processes due to the rotation of the solar core, radiative transfer zone, photosphere, chromosphere, and corona.

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