Hostname: page-component-77c89778f8-5wvtr Total loading time: 0 Render date: 2024-07-16T21:59:21.603Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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