Solar X-ray emission and metre-wave radio bursts

Details Solar X-ray emission and metre-wave radio bursts Solar X-ray emission and metre-wave radio bursts

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasau...3..154d&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 11th, Clayton, Victoria, Australia, May 30-June 1, 1977.) Astronomic

Astronomy and Astrophysics

Astronomy

2

Solar Corona, Solar Magnetic Field, Solar Radio Bursts, Solar X-Rays, Astronomical Maps, Solar Rotation, Spaceborne Astronomy, Spectroheliographs, Type 3 Bursts

Scientific paper

Scatter plots of the recorded positions of type I and type III solar radio bursts are compared with Skylab X-ray maps of the solar corona. The results suggest that radio bursts are nearly always close to bright X-ray regions, that X-ray-dull regions of the sun wider than 30 deg in longitude are almost completely free of radio bursts, that type I and type III activity apparently requires greater coronal disturbance than does X-ray emission, and that such activity is found only near the brightest X-ray regions. The 27-day recurrence pattern of the radio sources is briefly discussed.

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