The transformation of long scale Alfven waves in space dusty plasma

A nonlinear mechanism of the generation of kinetic Alfv´en waves (KAW) on dust plasma with small plasma parameter β is proposed. As the generation mechanism, the parametric instability where a pumping wave is the MHD Alfv´en wave is considered. On the basis of the three-fluid MHD, the nonlinear disp...

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Бібліографічні деталі
Опубліковано в: :Кинематика и физика небесных тел
Дата:2005
Автори: Yukhimuk, A.K., Fedun, V.M., Voitsekhovska, A.D., Cheremnykh, O.K.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
Теми:
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/79642
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:The transformation of long scale Alfven waves in space dusty plasma / A.K. Yukhimuk, V.M. Fedun, A.D. Voitsekhovska, O.K. Cheremnykh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 192-195. — Бібліогр.: 10 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79642
record_format dspace
spelling Yukhimuk, A.K.
Fedun, V.M.
Voitsekhovska, A.D.
Cheremnykh, O.K.
2015-04-03T16:59:48Z
2015-04-03T16:59:48Z
2005
The transformation of long scale Alfven waves in space dusty plasma / A.K. Yukhimuk, V.M. Fedun, A.D. Voitsekhovska, O.K. Cheremnykh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 192-195. — Бібліогр.: 10 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79642
A nonlinear mechanism of the generation of kinetic Alfv´en waves (KAW) on dust plasma with small plasma parameter β is proposed. As the generation mechanism, the parametric instability where a pumping wave is the MHD Alfv´en wave is considered. On the basis of the three-fluid MHD, the nonlinear dispersion equation describing the three-wave interaction is deduced and its solution is derived. Obtained instability growth rate is determined by parameters of dust plasma particles. The nonlinear process under consideration can take place both in laboratory and in space plasma with small plasma parameter β. As an application of theoretical results, we consider Saturn’s F-ring.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS2: Physics of Solar Atmosphere
The transformation of long scale Alfven waves in space dusty plasma
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title The transformation of long scale Alfven waves in space dusty plasma
spellingShingle The transformation of long scale Alfven waves in space dusty plasma
Yukhimuk, A.K.
Fedun, V.M.
Voitsekhovska, A.D.
Cheremnykh, O.K.
MS2: Physics of Solar Atmosphere
title_short The transformation of long scale Alfven waves in space dusty plasma
title_full The transformation of long scale Alfven waves in space dusty plasma
title_fullStr The transformation of long scale Alfven waves in space dusty plasma
title_full_unstemmed The transformation of long scale Alfven waves in space dusty plasma
title_sort transformation of long scale alfven waves in space dusty plasma
author Yukhimuk, A.K.
Fedun, V.M.
Voitsekhovska, A.D.
Cheremnykh, O.K.
author_facet Yukhimuk, A.K.
Fedun, V.M.
Voitsekhovska, A.D.
Cheremnykh, O.K.
topic MS2: Physics of Solar Atmosphere
topic_facet MS2: Physics of Solar Atmosphere
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description A nonlinear mechanism of the generation of kinetic Alfv´en waves (KAW) on dust plasma with small plasma parameter β is proposed. As the generation mechanism, the parametric instability where a pumping wave is the MHD Alfv´en wave is considered. On the basis of the three-fluid MHD, the nonlinear dispersion equation describing the three-wave interaction is deduced and its solution is derived. Obtained instability growth rate is determined by parameters of dust plasma particles. The nonlinear process under consideration can take place both in laboratory and in space plasma with small plasma parameter β. As an application of theoretical results, we consider Saturn’s F-ring.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79642
citation_txt The transformation of long scale Alfven waves in space dusty plasma / A.K. Yukhimuk, V.M. Fedun, A.D. Voitsekhovska, O.K. Cheremnykh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 192-195. — Бібліогр.: 10 назв. — англ.
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