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Title: | Perpendicularly propagating electromagnetic modes in a strongly magnetized hot plasma with non-Maxwellian distribution function |
Authors: | Zaheer, S. Murtaza, G. Shah, H. A. |
Issue Date: | 21-Jun-2006 |
Publisher: | Physics of plasmas |
Citation: | Zaheer, S., G. Murtaza, and H. A. Shah. "Perpendicularly propagating electromagnetic modes in a strongly magnetized hot plasma with non-Maxwellian distribution function." Physics of plasmas 13.6 (2006). |
Abstract: | Electromagnetic modes ordinary and extraordinary for strongly magnetized plasma are studied and their damping factors or and ex are calculated using non-Maxwellian velocity distribution function. It is observed that for moderate values of the spectral indices r and q used in r, q distribution functions , both the damping decrements show substantial change. As the value of the spectral index r increases for a fixed value of q, the damping increases for the O mode but decreases for the X mode. In the limiting case of r=0, q→ , the damping factors reduce to the standard Maxwellian values. © 2006 American Institute of Physics |
URI: | http://202.142.177.21/handle/123456789/2062 |
Appears in Collections: | Physics Department |
Files in This Item:
File | Description | Size | Format | |
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2006 Perpendicularly propagating electromagnetic modes in a strongly.pdf | 391.87 kB | Adobe PDF | View/Open |
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