The sun's outer corona at radio wavelengths

Details The sun's outer corona at radio wavelengths The sun's outer corona at radio wavelengths

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ijrsp..16..172k&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 16, Feb. 1987, p. 172-191. Research supported by NSF.

Astronomy and Astrophysics

Astronomy

3

Decametric Waves, Imaging Techniques, Radio Sources (Astronomy), Solar Corona, Astronomical Maps, Coronal Holes, Solar Radio Bursts, Spectroheliographs, Stellar Mass Ejection

Scientific paper

The use of meter-decameter wavelength imaging observations to follow four different kinds of studies of solar coronal activity is discussed. The Clark Lake Radio Observatory's multifrequency radioheliograph which operates in the 20-125 MHz frequency range is described. This paper emphasizes the differences observed in coronal phenomena with instruments having a higher sensitivity than the Culgoora instrument. New observations from the Clark Lake radioheliograph which show details of the long-lived structure of the corona are presented. These are then compared with features of the optical corona as shown in the data obtained by satellite-borne and ground-based coronagraphs.

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