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The Connection of Spectra with Other Pulsar Parameters

Published online by Cambridge University Press:  27 September 2017

Valerii M. Malofeev
Valerii M. Malofeev*
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute

Abstract

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An analysis has been made of the connection of characteristic frequencies and spectral indices with the following parameters of pulsars: P, Ṗ, T, L400, B, and χ. It is shown that a number of pulsar spectra apparently demonstrate the presence of two emission regions at a short distance between levels in the magnetosphere of pulsars, where the effects of the low-frequency turnover (LFT) and the high frequency cutoff (HFC) take place.

Type
Part IV Form and spectra of emission beams
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 157 - 160
Copyright
Copyright © United States Naval Observatory 1992