Observations of Bright Coronal Points at Wavelengths of 5.2 and 1.76 cm

Details Observations of Bright Coronal Points at Wavelengths of 5.2 and 1.76 cm Observations of Bright Coronal Points at Wavelengths of 5.2 and 1.76 cm

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001astl...27..181m&link_type=abstract

Astronomy Letters, vol. 27, p. 181-185 (2001)

Astronomy and Astrophysics

Astronomy

4

Sun, X-Ray Images, Coronal Points

Scientific paper

Based on two-dimensional solar images obtained with the Siberian Solar Radio Telescope and the Nobeyama Radio Heliograph and using YOHKOH soft X-ray images, we investigate bright coronal points. The principal microwave emission mechanism of these points is shown to be the thermal bremsstrahlung of an optically thin plasma. The fact that, in several cases, bright coronal points do not coincide at two wavelengths can be explained by imaging peculiarities of the Nobeyama Radio Heliograph rather than by physical factors.

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