Computer Science
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980m%26p....23..323p&link_type=abstract
Moon and the Planets, vol. 23, Nov. 1980, p. 323-338.
Computer Science
8
Comet Tails, Cometary Magnetospheres, Magnetospheres, Planetary Magnetospheres, Plasma Interactions, Solar Wind, Venus Atmosphere, Electrodynamics, Field Strength, Interplanetary Magnetic Fields, Plasma Interaction Experiment, Spatial Distribution, Three Dimensional Models
Scientific paper
The comparison of data obtained in laboratory experiments on the solar wind interaction with a body endowed with a plasma shell, the observations of comet type I tails and the direct measurements near Venus show that an induced magnetosphere is formed with an extended magnetic tail. This magnetosphere appears due to currents associated with unipolar induction. The distribution of electrodynamical forces associated with the formation of the induced magnetosphere makes it possible to explain the acceleration of matter towards the tail as in the motion across the tail observed in comets and Venus. The analysis of the condensation motion in Halley's comet yields an estimate of tail magnetic field of 30 to 50 gamma. A three-dimensional model of the induced magnetospheres of Venus and comets is developed.
Dubinin Edouard M.
Israelevich Peter L.
Podgorny I. M.
No associations
LandOfFree
Laboratory simulation of the induced magnetospheres of comets and Venus 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 Laboratory simulation of the induced magnetospheres of comets and Venus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Laboratory simulation of the induced magnetospheres of comets and Venus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1391751