Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases

Details Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37.1227c&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, Oct. 1989, p. 1227-1247.

Physics

Ampte (Satellites), Magnetosheath, Solar Wind, Boundary Layers, Electron Pressure, Magnetic Field Configurations, Magnetosonic Resonance, Photoionization, Pressure Gradients

Scientific paper

One-dimensional hybrid models are used to study the boundary layer structures that form at early times upstream of an AMPTE release in the solar wind or magnetosheath flow. The study emphasizes local interaction in terms of simple properties of supercritical, quasi-perpendicular shock transitions. The simulations are an extension of those of Chapman and Schwartz (1987) for the case of a release in the solar wind. The key features of the results are interpreted in terms of the ion kinetics and bulk plasma behavior of the transitions.

Affiliated with

Also associated with

No associations

Rating

Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases 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 Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Shocklike behaviour exhibited at early times by the AMPTE solar wind/magnetosheath releases will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1531898