Solar observations at 1.4 and 4.1 MM wavelengths with angular resolutions of 13 and 40 seconds of arc

Details Solar observations at 1.4 and 4.1 MM wavelengths with angular resolutions of 13 and 40 seconds of arc Solar observations at 1.4 and 4.1 MM wavelengths with angular resolutions of 13 and 40 seconds of arc

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pazh....1...24k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 1, Apr. 1975, p. 24-28. In Russian.

Astronomy and Astrophysics

Astronomy

1

Angular Resolution, Millimeter Waves, Solar Granulation, Solar Radio Emission, Chromosphere, Equators, Microwave Emission, Photosphere, Radio Astronomy

Scientific paper

Distributions of radio brightness for the equatorial zone of the sun obtained at 1,4 and 4,1 mm wavelengths with angular resolutions in right ascension of 14 and 40 seconds of arc show a number of small-scale features in solar regions devoid of corresponding optical details. This phenomenon is likely to be caused by chromospheric inhomogeneities analogous to photospheric granulation.

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