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Radio Physics and Radio Astronomy

Выходит 4 номеров в год

ISSN Печать: 2152-274X

ISSN Онлайн: 2152-2758

THE MECHANISM OF COMPONENT FORMATION OUT OF THE MAIN PULSE OF A RADIO PULSAR. II. THE INTERPULSE

Том 1, Выпуск 1, 2010, pp. 27-35
DOI: 10.1615/RadioPhysicsRadioAstronomy.v1.i1.40
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Краткое описание

The theory of induced scattering off the ultrarelativistic particles in a moderately strong magnetic field is developed. The kinetic equations obtained are applied to the problem of induced scattering of pulsar radiation out of the narrow beam. It is shown that the scattered radiation concentrates predominantly in the direction antiparallel to the velocity of the scattering particles. Based on this process, we first suggest a physical mechanism of the interpulse component of a pulsar. Our model explains the observed spectral and polarization peculiarities of the interpulse emission as well as its connection to the main pulse.

ЦИТИРОВАНО В
  1. Kontorovich V M, Trofymenko S V, Radiation reflection from star surface reveals the mystery of interpulse shift and appearance of high frequency components in the Crab pulsar, Journal of Physics: Conference Series, 932, 2017. Crossref

  2. Trofymenko S., Kontorovich V. M., Half-bare positron in the inner gap of a pulsar, Advances in Astronomy and Space Physics, 7, 1-2, 2017. Crossref

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