Depolarization of Pulsar Radio Emission

Astronomy and Astrophysics – Astrophysics

Scientific paper

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6 pages, 1 postscript figure

Scientific paper

10.1086/312335

We show that intensity dependent depolarization of single pulses (e.g.,
Xiluoris et al. 1994) may be due to the nonlinear decay of the "upper" ordinary
mode into an unpolarized extraordinary mode and a backward propagating wave.
The decay occurs in the innermost parts of the pulsar magnetosphere for
obliquely propagating O waves.

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