Some characteristics of S-component emission and bursts of solar emission at millimeter wavelengths

Details Some characteristics of S-component emission and bursts of solar emission at millimeter wavelengths Some characteristics of S-component emission and bursts of solar emission at millimeter wavelengths

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18...71m&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 71; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 2, Feb. 1992, p. 173-

Astronomy and Astrophysics

Astronomy

1

Microwave Emission, Millimeter Waves, Solar Flares, Solar Radio Bursts, Circular Polarization, Emission Spectra

Scientific paper

Simultaneous observations at wavelengths of 13 mm (parameters I and V) and 8 mm (I) resulted in the detection of correlations of the burst emission spectral index alphab with alpha of the parent local source and with burst rise time. The faster bursts have steeper spectra. The degree of circular polarization of the bursts does not exceed 35 percent, and the spectral index is in the range between -0.5 and -6.5. The burst characteristics observed may be explained via models of strongly inhomogeneous thermal sources or by a combination of both nonthermal and thermal radiation.

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