Direct evidence of type III electron streams propagating in coronal streamers

Details Direct evidence of type III electron streams propagating in coronal streamers Direct evidence of type III electron streams propagating in coronal streamers

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269l..67k&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 269, June 15, 1983, p. L67-L71.

Astronomy and Astrophysics

Astrophysics

23

Astronomical Photography, Solar Corona, Solar Electrons, Type 3 Bursts, Coronagraphs, Electron Density (Concentration), Solar Radio Emission, Spectroheliographs

Scientific paper

Using two-dimensional solar images at 73.8 MHz, obtained with the Clark Lake Multifrequency Radioheliograph, the authors present direct evidence that type III electron streams propagate in dense coronal streamers. This evidence is substantiated by the excellent coincidence that is found in position angle between the densest parts of streamers observed with the Solwind coronagraph on the P78-1 satellite and the maximum brightness of type III burst sources.

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