Optical identification of 1.35-cm-wavelength radio granulation with chromospheric-network elements

Details Optical identification of 1.35-cm-wavelength radio granulation with chromospheric-network elements Optical identification of 1.35-cm-wavelength radio granulation with chromospheric-network elements

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..550g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Dec. 1977, p. 550-553. In Russian.

Astronomy and Astrophysics

Astronomy

1

Chromosphere, Radio Astronomy, Solar Granulation, Solar Radio Emission, Brightness, Centimeter Waves, K Lines, Luminous Intensity

Scientific paper

Results are presented for simultaneous observations of the quiet-sun radio brightness distribution at a wavelength of 1.35 cm and the chromospheric network in the Ca II K line. Three pairs of radio and optical images are compared. It is found that practically all bright radio-granulation elements correspond to the most well-defined and brightest chromospheric-network vertices and that the most well-defined dark elements of the radio granulation coincide with well-defined dark inner-network fields of the chromospheric network (supergranule cell centers).

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