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Shock Waves and the Interpretation of the Chromospheric Calcium K-line

Published online by Cambridge University Press:  25 April 2016

L. E. Cram
L. E. Cram*
Affiliation:
Department of Applied Mathematics, University of Sydney
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Extract

Dissipation of shock waves has often been proposed as the energy source required to sustain the outward temperature rise in the solar atmosphere. Theoretical models for the heating process have been developed by equating the mechanical energy input to the radiative energy loss at each height, but neither of these processes is well understood, and the lack of data means that the models are necessarily crude.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 3 , October 1972 , pp. 146 - 147
Copyright
Copyright © Astronomical Society of Australia 1972

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References

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