Construction and Identification of Profiles of Curvature Radiation of Pulsars


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Abstract

Parameters of the observed radiation of pulsars are identified with the help of numerical simulation within the framework of the nonlinear least squares problem. With the help of the obtained parameter values, we have constructed profiles of radiation and indicatrices of the angular distribution of the instantaneous radiated power for experimentally observed pulsars.

About the authors

V. A. Avdyushev

National Research Tomsk State University

Author for correspondence.
Email: sch@niipmm.tsu.ru
Russian Federation, Tomsk

V. A. Bordovitsyn

National Research Tomsk State University

Email: sch@niipmm.tsu.ru
Russian Federation, Tomsk

A. A. Grokhovskaya

National Research Tomsk State University

Email: sch@niipmm.tsu.ru
Russian Federation, Tomsk

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