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Millimetre-wave second-harmonic generation in an underdense magnetoplasma in the presence of a magnetic wiggler

Published online by Cambridge University Press:  13 March 2009

Jetendra Parashar ,
H. D. Pandey ,
K. Ramachandran  and
R. K. Singh
Jetendra Parashar
Affiliation:
Centre for Energy Studies, Indian Institute of Technology, Delhi, New Delhi 110016, India
H. D. Pandey
Affiliation:
Physics Department, Barkatullah University, Bhopal 462028, India
K. Ramachandran
Affiliation:
Centre for Energy Studies, Indian Institute of Technology, Delhi, New Delhi 110016, India
R. K. Singh
Affiliation:
Centre for Energy Studies, Indian Institute of Technology, Delhi, New Delhi 110016, India
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Extract

A high-power millimetre wave (w1, k1) propagating through a magnetized plasma in the presence of a wiggler magnetic field (0, k0) produces density perturbations at (w1, K1 +K0). The density perturbations couple with the oscillatory velocity at (wl, K1) to produce a nonlinear current at (2w1, 2K1 +K0) driving second-harmonic electromagnetic radiation. The amplitude of the generated wave is sensitive to cyclotron resonance.

Type
Articles
Information
Journal of Plasma Physics , Volume 50 , Issue 2 , October 1993 , pp. 339 - 344
Copyright
Copyright © Cambridge University Press 1993

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