Three dimensional structure and time development of radio emission from solar active regions

Details Three dimensional structure and time development of radio emission from solar active regions Three dimensional structure and time development of radio emission from solar active regions

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983tuft.reptr....l&link_type=abstract

Final Report, 1 May 1980 - 31 Dec. 1982 Tufts Univ., Medford, MA. Dept. of Physics.

Physics

Brightness Temperature, Faculae, Solar Activity, Solar Radio Emission, Bremsstrahlung, Circular Polarization, Coronal Loops, Solar Magnetic Field

Scientific paper

The three dimensional structure of quiescent active regions was obtained by simultaneous multiple wavelength observations in the radio and optical parts of the spectrum. It is shown that the 6 cm radiation of solar active region is due to plage-associated bremsstrahlung and sunspot-associated gyroemission. The sunspot-associated component does not emit detectable X-ray radiation whereas the plage-associated component does. The dimensional structure of quiescent active regions and solar bursts; the slowly varying component of solar active region at 6 cm; the discovery of the radio wavelength counterpart of coronal loops observed at X-ray lengths; and multiple component bursts are discussed.

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