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

dc.contributor.author	Malov, I.F.
dc.contributor.author	Nikitina, E.B.
dc.date.accessioned	2017-06-04T18:56:39Z
dc.date.available	2017-06-04T18:56:39Z
dc.date.issued	2012
dc.description.abstract	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.	uk_UA
dc.description.sponsorship	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."	uk_UA
dc.identifier.citation	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.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	https://nasplib.isofts.kiev.ua/handle/123456789/119180
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.status	published earlier	uk_UA
dc.title	Distribution of areas of radiation generation at different frequencies in pulsar magnetospheres	uk_UA
dc.type	Article	uk_UA

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