On the structure of pulsar magnetospheres

The angles β between rotation and magnetic axes in the radio pulsar magnetospheres can be calculated with several methods. In this paper we present the results of calculations for three samples of radio pulsars at 10, 20 and 30 cm wavelength obtained with two methods using statistical relationships....

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Veröffentlicht in:Advances in Astronomy and Space Physics
Datum:2012
Hauptverfasser: Malov, I.F., Nikitina, E.B.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2012
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/119168
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Zitieren:On the structure of pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 28-30. — Бібліогр.: 4 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Malov, I.F.
Nikitina, E.B.
author_facet Malov, I.F.
Nikitina, E.B.
citation_txt On the structure of pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 28-30. — Бібліогр.: 4 назв. — англ.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
description The angles β between rotation and magnetic axes in the radio pulsar magnetospheres can be calculated with several methods. In this paper we present the results of calculations for three samples of radio pulsars at 10, 20 and 30 cm wavelength obtained with two methods using statistical relationships. Some effects which can give errors in the values of β are discussed. There are no correlations between values of β and pulsar ages.
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institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 2227-1481
language English
last_indexed 2025-12-07T20:41:53Z
publishDate 2012
publisher Головна астрономічна обсерваторія НАН України
record_format dspace
spelling Malov, I.F.
Nikitina, E.B.
2017-06-04T18:33:42Z
2017-06-04T18:33:42Z
2012
On the structure of pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 28-30. — Бібліогр.: 4 назв. — англ.
2227-1481
https://nasplib.isofts.kiev.ua/handle/123456789/119168
The angles β between rotation and magnetic axes in the radio pulsar magnetospheres can be calculated with several methods. In this paper we present the results of calculations for three samples of radio pulsars at 10, 20 and 30 cm wavelength obtained with two methods using statistical relationships. Some effects which can give errors in the values of β are discussed. There are no correlations between values of β and pulsar ages.
This work was supported by the Russian Foundation for Basic Research (project code 09-02-00584) and the Basic Research Program of the Presidium of the Russian Academy of Sciences on "The Origin, Structure, and Evolution of Objects in the Universe".
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
On the structure of pulsar magnetospheres
Article
published earlier
spellingShingle On the structure of pulsar magnetospheres
Malov, I.F.
Nikitina, E.B.
title On the structure of pulsar magnetospheres
title_full On the structure of pulsar magnetospheres
title_fullStr On the structure of pulsar magnetospheres
title_full_unstemmed On the structure of pulsar magnetospheres
title_short On the structure of pulsar magnetospheres
title_sort on the structure of pulsar magnetospheres
url https://nasplib.isofts.kiev.ua/handle/123456789/119168
work_keys_str_mv AT malovif onthestructureofpulsarmagnetospheres
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