A Mechanism For The Reversible Radio Emission in PSR B1822--09

Details A Mechanism For The Reversible Radio Emission in PSR B1822--09 A Mechanism For The Reversible Radio Emission in PSR B1822--09

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6b..81m&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S2, Proceedings of the 2005 Lake Hanas International

Astronomy and Astrophysics

Astrophysics

Pulsars: Radio Emission, Individual Psr B1822-09

Scientific paper

We discuss a possible scenario that allows explanation of the anti-correlation between MP sand IP of PSR B1822-09. We assume that the working regime of the inner gap is influenced by the outer gap. Depending on the surface temperature of the polar cap, one can expect alteration of the mean Lorentz factors of the secondary particles, which drastically affects the radio emission process. We also propose the model of generation of the coherent radio emission in reversible direction, toward the neutron star. The model is based on the resonant interaction of plasma clouds, created by gamma rays radiated in inner and outer gaps.

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