Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres

We analyse homogeneous samples of pulsars at 10 cm and 20 cm and propose to use n, the ratio of the half-width of the radiation cone θ to the minimum angular sight distance from the centre of this cone, to determine the levels of radiation generation at different frequencies in pulsar magnetospheres...

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Published in:Advances in Astronomy and Space Physics
Date:2012
Main Authors: Malov, I.F., Nikitina, E.B.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119180
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 125-127. — Бібліогр.: 6 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 Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 125-127. — Бібліогр.: 6 назв. — англ.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
description We analyse homogeneous samples of pulsars at 10 cm and 20 cm and propose to use n, the ratio of the half-width of the radiation cone θ to the minimum angular sight distance from the centre of this cone, to determine the levels of radiation generation at different frequencies in pulsar magnetospheres.
first_indexed 2025-12-07T18:43:56Z
format Article
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institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 2227-1481
language English
last_indexed 2025-12-07T18:43:56Z
publishDate 2012
publisher Головна астрономічна обсерваторія НАН України
record_format dspace
spelling Malov, I.F.
Nikitina, E.B.
2017-06-04T18:56:39Z
2017-06-04T18:56:39Z
2012
Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres / I.F. Malov, E.B. Nikitina // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 125-127. — Бібліогр.: 6 назв. — англ.
2227-1481
https://nasplib.isofts.kiev.ua/handle/123456789/119180
We analyse homogeneous samples of pulsars at 10 cm and 20 cm and propose to use n, the ratio of the half-width of the radiation cone θ to the minimum angular sight distance from the centre of this cone, to determine the levels of radiation generation at different frequencies in pulsar magnetospheres.
This work was financially supported by the Russian Foundation for Basic Research (project code 12-02-00661) and the Basic Research Program of the Presidium of the Russian Academy of Sciences "Nonsteady phenomena in the Universe."
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
Article
published earlier
spellingShingle Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
Malov, I.F.
Nikitina, E.B.
title Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
title_full Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
title_fullStr Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
title_full_unstemmed Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
title_short Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
title_sort distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
url https://nasplib.isofts.kiev.ua/handle/123456789/119180
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AT nikitinaeb distributionofareasofradiationgenerationatdifferentfrequenciesinpulsarmagnetospheres