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....
Збережено в:
| Дата: | 2012 |
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| Автори: | , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2012
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| Назва видання: | Advances in Astronomy and Space Physics |
| Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/119168 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
irk-123456789-119168 |
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| record_format |
dspace |
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irk-123456789-1191682017-06-05T03:03:58Z On the structure of pulsar magnetospheres Malov, I.F. Nikitina, E.B. 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. 2012 Article 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 http://dspace.nbuv.gov.ua/handle/123456789/119168 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| language |
English |
| 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. |
| format |
Article |
| author |
Malov, I.F. Nikitina, E.B. |
| spellingShingle |
Malov, I.F. Nikitina, E.B. On the structure of pulsar magnetospheres Advances in Astronomy and Space Physics |
| author_facet |
Malov, I.F. Nikitina, E.B. |
| author_sort |
Malov, I.F. |
| title |
On the structure of pulsar magnetospheres |
| 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 |
| publisher |
Головна астрономічна обсерваторія НАН України |
| publishDate |
2012 |
| url |
http://dspace.nbuv.gov.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. |
| series |
Advances in Astronomy and Space Physics |
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2023-10-18T20:33:55Z |
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2023-10-18T20:33:55Z |
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