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DC Field | Value | Language |
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dc.contributor.author | Zaheer, S. | - |
dc.contributor.author | Murtaza, G. | - |
dc.contributor.author | Shah, H. A. | - |
dc.date.accessioned | 2024-05-10T05:39:28Z | - |
dc.date.available | 2024-05-10T05:39:28Z | - |
dc.date.issued | 2006-06-21 | - |
dc.identifier.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). | en_US |
dc.identifier.other | DOI | - |
dc.identifier.uri | http://202.142.177.21/handle/123456789/2062 | - |
dc.description.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 | en_US |
dc.description.sponsorship | S. Zaheer acknowledges financial assistance from the Office of External Activities, Abdus Salam International Centre for Theoretical Physics, Trieste, Italy | en_US |
dc.language.iso | en_US | en_US |
dc.publisher | Physics of plasmas | en_US |
dc.title | Perpendicularly propagating electromagnetic modes in a strongly magnetized hot plasma with non-Maxwellian distribution function | en_US |
dc.type | Article | en_US |
Appears in Collections: | Physics Department |
Files in This Item:
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2006 Perpendicularly propagating electromagnetic modes in a strongly.pdf | 391.87 kB | Adobe PDF | View/Open |
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