Comparison of the 9.1 CM and soft X-ray emission from an active region

Details Comparison of the 9.1 CM and soft X-ray emission from an active region Comparison of the 9.1 CM and soft X-ray emission from an active region

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...48..121g&link_type=abstract

Solar Physics, vol. 48, May 1976, p. 121-125.

Astronomy and Astrophysics

Astronomy

7

Bremsstrahlung, Microwave Emission, Solar Radio Emission, Solar X-Rays, Superhigh Frequencies, Astronomical Maps, Brightness Temperature, Plasma Radiation, Radiation Measurement, Spaceborne Astronomy

Scientific paper

Thermal bremsstrahlung from the X-ray observed plasma accounts for most
of the observed 9.1 cm emission from McMath 12336, an old, spotless
active region, on June 2, 1973. This implies that only a small fraction
of the emission measure within the active region is in the range around
1,000,000 K and below.

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