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Corrected Formula for the Polarization of Second Harmonic Plasma Emission

Published online by Cambridge University Press:  25 April 2016

D. B. Melrose ,
G. A. Dulk  and
D. E. Gary
D. B. Melrose
Affiliation:
Department of Theoretical Physics, University of Sydney
G. A. Dulk
Affiliation:
Department of Astro-Geophysics, University of Colorado
D. E. Gary
Affiliation:
Department of Astro-Geophysics, University of Colorado
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Extract

Second harmonic plasma emission is attributed to the coalescence of two Langmuir waves into a transverse wave.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 50 - 53
Copyright
Copyright © Astronomical Society of Australia 1980

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References

Dulk, G. A., and McLean, D. J., Solar Phys., 57, 279 (1978).CrossRefGoogle Scholar
Melrose, R. B., Dulk, G. A., and Smerd, S. F., Astron. Astrophys., 66, 315 (1978).Google Scholar
Melrose, D. B., and Stenhouse, J. E., Astron. Astrophys., 73, 151 (1979).Google Scholar
Melrose, D. B., and Sy, W. N., Aust. J. Phys., 25, 387 (1972).CrossRefGoogle Scholar