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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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2012
Автори: Malov, I.F., Nikitina, E.B.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119180
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати: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.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119180
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
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
spellingShingle Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
Malov, I.F.
Nikitina, E.B.
title_short 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_sort distribution of areas of radiation generation at different frequencies in pulsar magnetospheres
author Malov, I.F.
Nikitina, E.B.
author_facet Malov, I.F.
Nikitina, E.B.
publishDate 2012
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
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.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119180
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.
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last_indexed 2025-12-07T18:43:56Z
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