Publication Abstracts
Canuto 1970
, 1970: Radiative opacities and Compton scattering in strong magnetic fields. Astrophys. J., 160, L153-L155, doi:10.1086/180549.
The Compton radiative opacity is computed in the presense of a strong magnetic field. It is found that the opacity along the magnetic field is decreased by a factor of (ω/ωH)2, where ωH is the cyclotron frequency, for both kinds of circular polarization. For the transverse opacity, half of the intensity is strongly absorbed when the electric field of the wave is parallel to H, while for the other half the opacity is rduced by the same factor of (ω/ωH)2.
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BibTeX Citation
@article{ca05500b,
author={Canuto, V.},
title={Radiative opacities and Compton scattering in strong magnetic fields},
year={1970},
journal={Astrophysical Journal},
volume={160},
pages={L153--L155},
doi={10.1086/180549},
}
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RIS Citation
TY - JOUR ID - ca05500b AU - Canuto, V. PY - 1970 TI - Radiative opacities and Compton scattering in strong magnetic fields JA - Astrophys. J. JO - Astrophysical Journal VL - 160 SP - L153 EP - L155 DO - 10.1086/180549 ER -
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