Backward Langmuir wave analysis and comparison with PIC simulation

Details Backward Langmuir wave analysis and comparison with PIC simulation Backward Langmuir wave analysis and comparison with PIC simulation

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pnaoc...3..203h&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 3, No.

Astronomy and Astrophysics

Astronomy

Langmuir Wave, Pic Simulation, Thermal Velocity

Scientific paper

Langmuir waves converted into electromagnetic radiation is an important mechanism of solar typye III bursts. Langmuir waves can be easily excited by electron beam instability. Generally, the second harmonic waves are produced through coalescence of the forward and backward propagating Langmuir waves. In this apper, the equations of two stream instability are resolved with the thermal velocity, and it is found that the dispersion relation of the forward propagating Langmuir wave depends on the drift speed, and the backward propagating Langmuir wave depends on the thermal velocity. Same conclusions have been confirmed by PIC simulations.

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