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A model of the inner corona based on radio data

Published online by Cambridge University Press:  14 August 2015

B. N. Panovkin
B. N. Panovkin*
Affiliation:
Academy of Sciences, Moscow, U.S.S.R.

Extract

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The work of Ginzburg, Shklovskiĭ, and Martyn (1946) showed that the upper layers of the solar atmosphere (chromosphere and corona) are responsible for the sun's thermal emission in the radio-emission range. This was confirmed by a number of observations.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 105 - 106
Copyright
Copyright © Stanford University Press 1959