Quantized electromagnetic tornado in pulsar vacuum gap

Abstract

The solution for the electromagnetic tornado in a vacuum gap of a pulsar that could serve as an explanation of the observed circular polarization of giant pulses from pulsars and might also explain the frequency strips observed in giant pulses spectrum is found.

4 pages, 3 Postscript figures; The fifth International conference Solitons, collapses and turbulence: achivement, developments and perspectives, dedicated to the 70-th anniversary of Professor Vladimir Zakharov, ed. E.A.Kuznetsov, Chernogolovka: ITP RAS, p.24 (2009)

References in corpus (1)

• Giant Pulses from PSR B1937+21 with widths <= 15 nanoseconds and T_b >= 5 x 10^39 K, the Highest Brightness Temperature Observed in the Universe

Cited by in corpus (1)

• On high brightness temperature of pulsar giant pulses