Spatial and spectral structure of a solar flaring loop at centimeter wavelengths

Details Spatial and spectral structure of a solar flaring loop at centimeter wavelengths Spatial and spectral structure of a solar flaring loop at centimeter wavelengths

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...191..365p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 191, no. 2, Feb. 1988, p. 365-373.

Astronomy and Astrophysics

Astrophysics

18

Centimeter Waves, Solar Flares, Solar Radio Bursts, Solar Spectra, Brightness Temperature, Circular Polarization, Optical Thickness, Solar Magnetic Field, Synchrotron Radiation

Scientific paper

The authors have studied the behaviour of the gyrosynchrotron emission coefficient and source function as a function of the strength and direction of the magnetic field. The results are applied in the qualitative description of the spatial and spectral structure of solar microwave bursts. In addition the authors present a complete set of model computations of microwave emission from a loop filled with energetic electrons. Their model predicts footpoint emission at short wavelengths and emission from the entire loop at long wavelengths. The computed spectra of the emission show considerable variation along the flaring loop.

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