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

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

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kfnt...10...58v&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 10, No. 1, p. 58 - 60

Physics

Cometary Plasma: Structure, Cometary Tails: Structure, Cometary Tails: Filaments, Cometary Tails: Solar Wind

Scientific paper

The theoretical model of large-scale ray structure formation proposed in the preceding paper consists in the development of filamentation instability due to the solar wind flow penetrating into a cometary plasma tail. In order to investigate the real form of the filaments and instability development in space, a study of the proposed mechanism in three dimensions is made. The cometary plasma filaments, which are observed as bright rays, are formed due to instability development and take the form of cylindrical plasma fibers with thickness determined by cometary plasma parameters and those of the solar wind.

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