Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 278, Issue 1-2, Pages 77-80Publisher
KLUWER ACADEMIC PUBL
DOI: 10.1023/A:1013183218726
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We have developed a numerical code for the propagation of different electromagnetic modes in a pulsar magnetosphere filled by a relativistic, streaming electron-positron plasma in a strong, curved magnetic field. We determine the trajectories, limiting polarization and damping of the waves leaving the magnetosphere.
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