The spectrum of coronal sources at millimetre and centimetre waves

Details The spectrum of coronal sources at millimetre and centimetre waves The spectrum of coronal sources at millimetre and centimetre waves

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..124..157b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 124, no. 1, 1989, p. 157-166.

Physics

7

Brightness Temperature, Millimeter Waves, Solar Corona, Solar Magnetic Field, Solar Radio Emission, Centimeter Waves, Polarization (Waves)

Scientific paper

Recently recognized solar mm-wave off-limb sources are interpreted as a special phenomenon of long-duration post- and inter-flare emission at coronal altitudes. Information about the brightness and polarization spectrum in the cm range is given for such an event on September 22, 1980. The brightness temperatures observed favor the interpretation of the bulk of the emission by thermal optically thin bremsstrahlung.

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