Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..91..167k&link_type=abstract
Astrophysics and Space Science (ISSN 0004-040X), vol. 91, no. 1, March 1983, p. 167-214.
Astronomy and Astrophysics
Astrophysics
30
Plasma Diffusion, Plasma Radiation, Pulsars, Radiation Spectra, Spectrum Analysis, Gamma Ray Spectra, Magnetic Flux, Plasma Density, Plasma Temperature, Radiant Flux Density, X Ray Spectra
Scientific paper
The spectra of outgoing radiation are treated. It is pointed out that the results of Meszaros and Bonazzola (1981) on this topic differ markedly from those at Kaminker et al. (1983) and Silant'ev (1980, 1982). The difference is thought to be due to the low accuracy of the calculations by Meszaros and Bonazzola for semi-infinite plasma. The basic formulas of the coupled diffusion method are presented and analyzed for different magnitudes of the transfer coefficients. The spectra of certain fluxes of the outgoing radiation are investigated, along with their dependence on the magnetic field, density and temperature. Attention is also given to the directional dependence of the intensity and polarization spectra. The effects of finite plasma thickness, inhomogeneity of density and temperature, departure from local thermodynamical equilibrium and Comptonization are discussed.
Kaminker A. D.
Pavlov George G.
Shibanov Iu. A.
No associations
LandOfFree
Spectra of radiation from a strongly magnetized plasma 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 Spectra of radiation from a strongly magnetized plasma, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectra of radiation from a strongly magnetized plasma will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1465776