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Coronal Density Structures in Regions of Type III Activity

Published online by Cambridge University Press:  25 May 2016

Yolande Leblanc
Affiliation:
Observatoire de Meudon, France
Thomas B. H. Kuiper*
Affiliation:
University of Maryland, U.S.A.
Shirley Hansen
Affiliation:
High Altitude Observatory, U.S.A.
*
*Present address: Jet Propulsion Laboratory, 183 B-365, California Institute of Technology, Pasadena, Calif. 91103, U.S.A.

Abstract

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(Solar Phys.). We identify from daily K-corona observations the coronal regions located above type III burst sources. The radio observations were made with the east–west log-periodic array at Clark Lake Observatory. East–west positions of 260 isolated type III bursts during March and April 1971 have been measured between 20 and 65 MHz (disregarding storms of type III bursts). The K-corona observations are made with the HAO K-coronameter at Mauna Loa, Hawaii. During 1971, the heights of observation were 3.6′, 5′, 9′ and 13′ above the limb.

Type
Part II The Flash Phase of Solar Flares
Copyright
Copyright © Reidel 1974