The magnetic field of the plasma tail of Comet 1P/Halley

The photometric scans of the plasma tail of Comet Halley from four observation series are compared with the profiles of brightness distribution along the tail streams which were calculated on the basis of the diffusion model of the plasma tail. The magnetic field induction and the lifetime of ions i...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
1. Verfasser: Sizonenko, Yu.V.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79706
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Zitieren:The magnetic field of the plasma tail of Comet 1P/Halley / Yu.V. Sizonenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 491-493. — Бібліогр.: 5 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Sizonenko, Yu.V.
author_facet Sizonenko, Yu.V.
citation_txt The magnetic field of the plasma tail of Comet 1P/Halley / Yu.V. Sizonenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 491-493. — Бібліогр.: 5 назв. — англ.
collection DSpace DC
container_title Кинематика и физика небесных тел
description The photometric scans of the plasma tail of Comet Halley from four observation series are compared with the profiles of brightness distribution along the tail streams which were calculated on the basis of the diffusion model of the plasma tail. The magnetic field induction and the lifetime of ions in the tail of Comet Halley as well as the coefficients of diffusion are estimated. A probable connection between cometary magnetic field changes and cometary tail structure ones are discussed.
first_indexed 2025-12-07T16:45:47Z
format Article
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id nasplib_isofts_kiev_ua-123456789-79706
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 0233-7665
language English
last_indexed 2025-12-07T16:45:47Z
publishDate 2005
publisher Головна астрономічна обсерваторія НАН України
record_format dspace
spelling Sizonenko, Yu.V.
2015-04-03T19:54:24Z
2015-04-03T19:54:24Z
2005
The magnetic field of the plasma tail of Comet 1P/Halley / Yu.V. Sizonenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 491-493. — Бібліогр.: 5 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79706
The photometric scans of the plasma tail of Comet Halley from four observation series are compared with the profiles of brightness distribution along the tail streams which were calculated on the basis of the diffusion model of the plasma tail. The magnetic field induction and the lifetime of ions in the tail of Comet Halley as well as the coefficients of diffusion are estimated. A probable connection between cometary magnetic field changes and cometary tail structure ones are discussed.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS5: Dynamics and Physics of Solar System Bodies
The magnetic field of the plasma tail of Comet 1P/Halley
Article
published earlier
spellingShingle The magnetic field of the plasma tail of Comet 1P/Halley
Sizonenko, Yu.V.
MS5: Dynamics and Physics of Solar System Bodies
title The magnetic field of the plasma tail of Comet 1P/Halley
title_full The magnetic field of the plasma tail of Comet 1P/Halley
title_fullStr The magnetic field of the plasma tail of Comet 1P/Halley
title_full_unstemmed The magnetic field of the plasma tail of Comet 1P/Halley
title_short The magnetic field of the plasma tail of Comet 1P/Halley
title_sort magnetic field of the plasma tail of comet 1p/halley
topic MS5: Dynamics and Physics of Solar System Bodies
topic_facet MS5: Dynamics and Physics of Solar System Bodies
url https://nasplib.isofts.kiev.ua/handle/123456789/79706
work_keys_str_mv AT sizonenkoyuv themagneticfieldoftheplasmatailofcomet1phalley
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