Propagation of high-frequency electromagnetic waves through a magnetized plasma in curved space-time
Creators
- 1. Max-Planck-Institut fuer Physik und Astrophysik, Muenchen (Germany, F.R.)
Description
This is the second of two papers on the propagation of high-frequency electromagnetic waves through an inhomogeneous, non-stationary plasma in curved space-time. By applying the general two-scale W.K.B. method developed in part 1 to the basic wave equation, derived also in that paper, the dispersion relation, the rays, the polarization states and the transport laws for the amplitudes of these waves are observed. In a magnetized plasma the polarization state changes differently for ordinary and extraordinary waves, according to the angle between the wave-normal and the background magnetic field, and under specified approximation conditions the direction of polarization of linearly polarized waves undergoes a generalized Faraday rotation. (author)
Additional details
Additional titles
- Subtitle (English)
- 2. Application of the asymptotic approximation
Publishing Information
- Journal Title
- Proc. R. Soc. (London), Ser. A
- Journal Volume
- 374
- Journal Issue
- 1756
- Series
- Proc. R. Soc. (London), Ser. A.
- Journal Page Range
- 65-86
- ISSN
- 0080-4630
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 12593991
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMPLITUDES; BOUNDARY CONDITIONS; DISPERSION RELATIONS; ELECTROMAGNETIC RADIATION; FARADAY EFFECT; FREQUENCY RANGE; INHOMOGENEOUS PLASMA; MAGNETIC FIELDS; NEUTRON STARS; PERTURBATION THEORY; POLARIZATION; SPACE-TIME; STAR ACCRETION; TRANSPORT THEORY; WAVE FUNCTIONS; WAVE PROPAGATION
- Descriptors DEC
- FUNCTIONS; PLASMA; RADIATIONS; STAR EVOLUTION; STARS