COMPARISON OF CORONAL STRUCTURE DEDUCED FROM FARADAY ROTATION MEASUREMENTS WITH SOLAR RADIO MAPS AT 2.8 AND 11 CM

Publisher Website

1 January 1978

book chapter
Published by Elsevier

p. 377-380
https://doi.org/10.1016/b978-0-08-022021-5.50085-9

Abstract

No abstract available

Keywords

This publication has 3 references indexed in Scilit:

A coronal hole observed at 10.7 GHz with a large single dish
Solar Physics, 1975
Inferring the interplanetary magnetic field by observing the polar geomagnetic field
Reviews of Geophysics, 1972
The quasi-stationary coronal magnetic field and electron density as determined from a Faraday rotation experiment
Solar Physics, 1970