Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping

Details Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.174..217c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 174, no. 2, Dec. 1990, p. 217-228.

Statistics

Computation

3

Neutron Stars, Stellar Magnetic Fields, Thomson Scattering, White Dwarf Stars, Compton Effect, Computational Astrophysics, Damping, Electron Cyclotron Heating, Electron Gas, Stellar Radiation, Wave Scattering

Scientific paper

The effect of a strong magnetic field on Thomson scattering is investigated taking into account radiation damping by using the Abraham-Lorentz equation instead of the Newton-Lorentz equation. The Stokes parameters for Thomson scattering are computed in terms of the state of polarization of the incident wave, the electron-cyclotron frequency, the angle of incidence, and the angle of scattering. It is noted that the Stokes parameters for the scattered radiation show resonance structures.

Affiliated with

Also associated with

No associations

Rating

Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping 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 Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stokes parameters for Thomson scattering in a strong magnetic field with radiation damping will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1629254