A simple solar microwave burst observed with high spectral resolution

Details A simple solar microwave burst observed with high spectral resolution A simple solar microwave burst observed with high spectral resolution

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339.1115g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 1115-1122.

Astronomy and Astrophysics

Astrophysics

13

Microwave Spectra, Solar Flares, Solar Radio Bursts, Solar Spectra, Interferometry, Microwave Emission, Power Spectra, Radio Spectra, Solar Magnetic Field, Spectral Resolution

Scientific paper

A small flare that occurred on February 3, 1986 which was dominated by a
single homogeneous source is analyzed. The theory of microwave emission
from homogeneous sources was used to trace the evolution of the burst.
The spectral profile indicates a thermal origin. It was found that the
source expanded with time during the burst.

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