A linear model of formation of ray structures in a cometary plasma tail

The theoretical model of large-scale ray structure formation proposed in the preceding paper resides in the filamentation instability development due to the solar wind flow penetrating into the cometary plasma tail. In order to investigate a real form of the filaments and instability development in...

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Bibliographic Details
Published in:Кинематика и физика небесных тел
Date:1994
Main Author: Verkhoglyadova, O.P.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 1994
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/214974
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:A linear model of formation of ray structures in a cometary plasma tail / O.P. Verkhoglyadova // Кинематика и физика небесных тел. — 1994. — Т. 10, № 1. — С. 58-60. — Бібліогр.: 8 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine