Direct evidence of type III electron streams propagating in coronal streamers

Journal Article · Wed Jun 15 00:00:00 EDT 1983 · Astrophys. J., Lett. Ed.; (United States)

DOI:https://doi.org/10.1086/184057· OSTI ID:5890152

Kundu, M R; Gergely, T E; Turner, P J; Howard, R A

Using two-dimensional solar images at 73.8 MHz, obtained with the Clark Lake Multifrequency Radioheliograph, we present direct evidence that type III electron streams propagate in dense coronal streamers. This evidence is substantiated by the excellent coincidence that we find 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.

• Research Organization: Astronomy Program, Clark Lake Radio Observatory, University of Maryland
• OSTI ID: 5890152
• Journal Information: Astrophys. J., Lett. Ed.; (United States), Vol. 269:2
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SOLAR CORONA
ELECTRON BEAMS
SOLAR RADIO BURSTS
MHZ RANGE 01-100
BEAMS
ELECTROMAGNETIC RADIATION
FREQUENCY RANGE
LEPTON BEAMS
MHZ RANGE
PARTICLE BEAMS
RADIATIONS
RADIOWAVE RADIATION
SOLAR ACTIVITY
640104* - Astrophysics & Cosmology- Solar Phenomena