A coronal hole observed at 10.7 GHz with a large single dish

Details A coronal hole observed at 10.7 GHz with a large single dish A coronal hole observed at 10.7 GHz with a large single dish

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..157f&link_type=abstract

Solar Physics, vol. 42, May 1975, p. 157-161. Research supported by the Deutsche Forschungsgemeinschaft.

Physics

15

Brightness Temperature, Electron Density (Concentration), Microwave Emission, Solar Corona, Solar Radio Emission, Astronomical Maps, Far Ultraviolet Radiation, Line Spectra, Radiant Flux Density

Scientific paper

On July 24, 1973, a coronal hole was observed at 10.69 GHz (2.8 cm) with
the Bonn 100-m telescope. The difference between brightness temperatures
measured outside and inside the hole was about 400 to 500 K. It is shown
that this lack of emission can be explained by usually adopted values of
the electron density at the bottom of the corona.

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