Canuto et al. 1971
Canuto, V., J. Lodenquai, and M. Ruderman, 1971: Thomson scattering in a strong magnetic field. Phys. Rev. D, 3, 2303-2308, doi:10.1103/PhysRevD.3.2303.
The effect of a strong magnetic field on neutron stars or white dwarfs is calculated for Thomson scattering in a fully ionized collisionless plasma. The photon mean free path can be greatly extended for propagation nearly parallel or, for the extraordinary mode, nearly perpendicular to the field.
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Canuto, V., Lodenquai, J., and Ruderman, M.: Thomson scattering in a strong magnetic field, Phys. Rev. D, 3, 2303-2308, doi:10.1103/PhysRevD.3.2303, 1971.
Canuto, V., J. Lodenquai, and M. Ruderman (1971), Thomson scattering in a strong magnetic field, Phys. Rev. D, 3, 2303-2308, doi:10.1103/PhysRevD.3.2303.
Canuto, V., J. Lodenquai, and M. Ruderman, 1971: Thomson scattering in a strong magnetic field. Phys. Rev. D, 3, 2303-2308, doi:10.1103/PhysRevD.3.2303.
Canuto, V., Lodenquai, J., & Ruderman, M. 1971, Phys. Rev. D, 3, 2303, doi:10.1103/PhysRevD.3.2303.
Canuto V, Lodenquai J, Ruderman M. Thomson scattering in a strong magnetic field, Phys Rev D 1971;3:2303-2308. doi:10.1103/PhysRevD.3.2303.
V. Canuto, J. Lodenquai, M. Ruderman, Phys. Rev. D 3, 2303-2308, doi:10.1103/PhysRevD.3.2303 (1971).
