On the structure of pulsar magnetospheres

Домашня сторінка
→
Фізико-технічні та математичні науки
→
Відділення фізики і астрономії
→
Advances in Astronomy and Space Physics
→
Advances in Astronomy and Space Physics, 2012, том 2
→
Advances in Astronomy and Space Physics, 2012, вип. 1
→
Переглянути статтю

dc.contributor.author	Malov, I.F.
dc.contributor.author	Nikitina, E.B.
dc.date.accessioned	2017-06-04T18:33:42Z
dc.date.available	2017-06-04T18:33:42Z
dc.date.issued	2012
dc.identifier.citation	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.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119168
dc.description.abstract	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.	uk_UA
dc.description.sponsorship	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".	uk_UA
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.title	On the structure of pulsar magnetospheres	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA