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=1990scsmp..33..446l&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 0253-5831), vol. 33, April 1990, p

Mathematics

Logic

2

Comet Tails, Magnetic Field Configurations, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Solar Wind, Plasma-Electromagnetic Interaction, Roots Of Equations, Vortices

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 analyzed. Based on the theories of magnetic hydrodynamics and force-free 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.

Affiliated with

Also associated with

No associations

Rating

Disturbance structures and their magnetic field features in plasma comet tail does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Disturbance structures and their magnetic field features in plasma comet tail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Disturbance structures and their magnetic field features in plasma comet tail will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1383518