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Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range

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Title: Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range
Authors: Ulyanov, O. M., Skoryk, A. O., Shevtsova, A. I., Plakhov, M. S., Ulyanova, O. O.
Publication Year: 2015
Collection: Astrophysics
Subject Terms: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
More Details: In this paper the anomalous intense pulse of the PSR J0953+0755 was studied in decametre wavelength range. For this pulse two scales of fine structure were discovered. The long-scale structure consists of four components, where the visible dispersion measures of even and odd components are different. The obtained time-scale of the short fine structure is 1 ms. The difference in visible dispersion measure can be caused by propagation of two normal modes of the pulsar radiation and irregularities of electron concentration in the space near the neutron star like upper layers of magnetosphere and pulsar wind.
Comment: 9 pages, 7 figures
Document Type: Working Paper
DOI: 10.1093/mnras/stv2172
Access URL: http://arxiv.org/abs/1510.02815
Accession Number: edsarx.1510.02815
Database: arXiv
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  Data: Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range
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  Data: <searchLink fieldCode="AR" term="%22Ulyanov%2C+O%2E+M%2E%22">Ulyanov, O. M.</searchLink><br /><searchLink fieldCode="AR" term="%22Skoryk%2C+A%2E+O%2E%22">Skoryk, A. O.</searchLink><br /><searchLink fieldCode="AR" term="%22Shevtsova%2C+A%2E+I%2E%22">Shevtsova, A. I.</searchLink><br /><searchLink fieldCode="AR" term="%22Plakhov%2C+M%2E+S%2E%22">Plakhov, M. S.</searchLink><br /><searchLink fieldCode="AR" term="%22Ulyanova%2C+O%2E+O%2E%22">Ulyanova, O. O.</searchLink>
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  Data: 2015
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– Name: Abstract
  Label: Description
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  Data: In this paper the anomalous intense pulse of the PSR J0953+0755 was studied in decametre wavelength range. For this pulse two scales of fine structure were discovered. The long-scale structure consists of four components, where the visible dispersion measures of even and odd components are different. The obtained time-scale of the short fine structure is 1 ms. The difference in visible dispersion measure can be caused by propagation of two normal modes of the pulsar radiation and irregularities of electron concentration in the space near the neutron star like upper layers of magnetosphere and pulsar wind.<br />Comment: 9 pages, 7 figures
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  Data: 10.1093/mnras/stv2172
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      – SubjectFull: Astrophysics - Solar and Stellar Astrophysics
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      – TitleFull: Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range
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            NameFull: Skoryk, A. O.
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            NameFull: Shevtsova, A. I.
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            NameFull: Plakhov, M. S.
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