Disturbance structures and their magnetic field features in plasma comet tail.

Details Disturbance structures and their magnetic field features in plasma comet tail. Disturbance structures and their magnetic field features in plasma comet tail.

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990scisn..33..446l&link_type=abstract

Scientia Sinica, Ser. A, Vol. 33, No. 4, p. 446 - 453

Physics

Cometary Tails: Solar Wind, Cometary Plasma: Magnetohydrodynamics

Scientific paper

The solar wind disturbances result in the emergence of condensation structures in plasma comet tails. Most of them are correlated with plasma vortex flows. The features of condensations are analysed. Based on the theories of magnetic hydrodynamics and forcefree fields, the construction and the distribution of magnetic field and its energy in condensations are specifically discussed. Details on the coupling process between an unsteady plasma motion and a magnetic field are given.

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