On the structure of pulsar magnetospheres
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....
Saved in:
| Published in: | Advances in Astronomy and Space Physics |
|---|---|
| Date: | 2012 |
| Main Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2012
|
| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/119168 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | 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. |
Institution
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-119168 |
|---|---|
| record_format |
dspace |
| spelling |
Malov, I.F. Nikitina, E.B. 2017-06-04T18:33:42Z 2017-06-04T18:33:42Z 2012 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. 2227-1481 https://nasplib.isofts.kiev.ua/handle/123456789/119168 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. 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". en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics On the structure of pulsar magnetospheres Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
On the structure of pulsar magnetospheres |
| spellingShingle |
On the structure of pulsar magnetospheres Malov, I.F. Nikitina, E.B. |
| title_short |
On the structure of pulsar magnetospheres |
| title_full |
On the structure of pulsar magnetospheres |
| title_fullStr |
On the structure of pulsar magnetospheres |
| title_full_unstemmed |
On the structure of pulsar magnetospheres |
| title_sort |
on the structure of 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 |
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.
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119168 |
| citation_txt |
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. |
| work_keys_str_mv |
AT malovif onthestructureofpulsarmagnetospheres AT nikitinaeb onthestructureofpulsarmagnetospheres |
| first_indexed |
2025-12-07T20:41:53Z |
| last_indexed |
2025-12-07T20:41:53Z |
| _version_ |
1850883560083292160 |