A model for solar oscillations at CM and MM wavelengths

Details A model for solar oscillations at CM and MM wavelengths A model for solar oscillations at CM and MM wavelengths

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...48...85s&link_type=abstract

Solar Physics, vol. 48, May 1976, p. 85-87. Research supported by the National Research Council of Canada.

Physics

Electron Density Profiles, Electron Energy, Plasma Oscillations, Solar Electrons, Stellar Models, Electron Oscillations, Millimeter Waves, Plasma Frequencies, Solar Atmosphere, Superhigh Frequencies, Thermal Radiation

Scientific paper

It is suggested that large scale oscillations of the sun give rise to the periodic fluctuations observed in the quiet sun at radio wavelengths. These fluctuations would be most readily observed from regions where there is a large gradient of electron temperature with electron density, and are thus more readily observed at cm wavelengths than at millimeter wavelengths.

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