Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..229f&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 2, March 1989, p. 229-251.
Astronomy and Astrophysics
Astrophysics
1
Anisotropic Media, Cerenkov Radiation, Plasma Radiation, Charge Transfer, Far Fields, Magnetic Fields, Propagation Modes, Whistlers
Scientific paper
Following a series of works on anisotropic radiation, the Cerenkov condition in magnetized plasmas is analyzed. It is discovered that the usual Cerenkov condition cos theta = 1/n beta(parallel) is not satisfied at a far field point in anisotropic media, implying that, when a charge is moving in a magnetized plasma, a linear shock wave front does not form. Thus, the power received at a far field per unit time in such a medium can be calculated; this quantity could not be evaluated according to previous theory. Numerical examples are presented to show various relevant characteristics of Cerenkov radiation in model plasmas.
Fung C. W. P.
Leung P. L.
No associations
LandOfFree
Cerenkov radiation in anisotropic plasmas does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cerenkov radiation in anisotropic plasmas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cerenkov radiation in anisotropic plasmas will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1801422