On the structure of pulsar magnetospheres
| 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.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.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 | https://nasplib.isofts.kiev.ua/handle/123456789/119168 | |
| 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 | On the structure of pulsar magnetospheres | uk_UA |
| dc.type | Article | uk_UA |
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