Electromagnetic theory of collisional interchange instabilities

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Atmospheric Electricity, Electric Fields, Electromagnetic Interactions, Ionospheric Disturbances, Space Plasmas, Barium Ion Clouds, Collisional Plasmas, Ionospheric Currents, Plasma Density, Spread F

Scientific paper

Finite parallel wavelength is shown to have a significant effect on the linear growth of instabilities of the Rayleigh-Taylor or E x B gradient drift types. The flute approximation, which explicitly neglects electric fields parallel to the ambient magnetic field, is asymptotically correct for long perpendicular wavelengths, if the parallel component of the electric field is primarily inductive in character. However, when the parallel electric field is primarily electrostatic, there is a profound reduction in the growth rate for long perpendicular wavelengths. This reduction in growth rate arises because parallel electron currents short-circuit the perpendicular electric field driving the instability. Parallel electric fields are more likely to be electrostatic in lower-density plasmas than in higher-density plasmas. Consequently, the extrapolation of structuring from low-density plasmas, such as those found in the spread-F environment, to higher-density ionospheric plasmas may not be reasonable.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Electromagnetic theory of collisional interchange instabilities 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 Electromagnetic theory of collisional interchange instabilities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electromagnetic theory of collisional interchange instabilities will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1803839

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.