Origin of quasi-harmonic emission bands with fine structure in the dynamic spectra of high-frequency interpulses of the Crab pulsar. Issue 4 (23rd May 2020)

• Record Type: Journal Article
• Authors: Zheleznyakov, V V; Shaposhnikov, V E
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 495:Issue 4(2020)
• Page Start: 3715
• Page End: 3721
• Publication Date: 2020-05-23
• Subjects: radiation mechanisms: non-thermal -- methods: analytical -- pulsars: individual: NP0532; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa1424
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We study the origin of quasi-harmonic emission bands with fine structure observed in the dynamic radiation spectra of high-frequency interpulses. The possible explanation of observed structure is based on the effect of double plasma resonance (DPR) at electron cyclotron harmonics realized in the magnetosphere of pulsar in a local radio emission source filled with non-relativistic plasma. The model of the source consists of neutral current sheet with a transverse magnetic field where plasma waves are generated due to DPR effect. It is shown that the emergence of emission bands and their frequency spacing are due to the inhomogeneity of the plasma and magnetic field along the current sheet, and their fine structure is due to the inhomogeneity of the current sheet in the direction orthogonal to it. Each quasi-harmonic emission band represents a system of elements of fine features of radiation that is generated by suprathermal electrons under DPR conditions. The observed upward drift of quasi-harmonic emission bands is due to the displacement of suprathermal electrons across the current sheet and an increase in the DPR frequencies with distance from the central plane of the layer.