Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-02-08
Astrophys.Space Sci. 262 (1999) 379-389
Astronomy and Astrophysics
Astrophysics
11 pages, LaTeX
Scientific paper
10.1023/A:1001872805645
We consider the polarization behaviour of radio waves propagating through an ultrarelativistic highly magnetized electron-positron plasma in a pulsar magnetosphere. The rotation of magnetosphere gives rise to the wave mode coupling in the polarization-limiting region. The process is shown to cause considerable circular polarization in the linearly polarized normal waves. Thus, the circular polarization observed for a number of pulsars, despite the linear polarization of the emitted normal waves, can be attributed to the limiting-polarization effect.
Lyubarskii Y. E.
Petrova S. A.
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