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A model of the inner corona based on radio data
Published online by Cambridge University Press: 14 August 2015
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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
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