Bi-ion fluid description of plasma dust interaction: relevance to Phobos events.

Details Bi-ion fluid description of plasma dust interaction: relevance to Phobos events. Bi-ion fluid description of plasma dust interaction: relevance to Phobos events.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13q.291b&link_type=abstract

Advances in Space Research, Vol. 13, No. 10, p. 291 - 294

Physics

3

Scientific paper

Significant magnetic field and plasma perturbations in the solar wind were observed during the Phobos-2 elliptical orbits around Mars at the Phobos orbit crossings (Phobos events). As a remarkable feature, the perturbations were detected in all cases on the upstream side of the Phobos orbit. The authors present a simple theory of solar wind-dust interaction on the basis of a Hall-MHD plasma model, and suggest the Phobos events to be the signatures of phase-standing waves excited in the solar wind upstream of a thin charged dust torus along the Phobos orbit.

Affiliated with

Also associated with

No associations

Rating

Bi-ion fluid description of plasma dust interaction: relevance to Phobos events. 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 Bi-ion fluid description of plasma dust interaction: relevance to Phobos events., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bi-ion fluid description of plasma dust interaction: relevance to Phobos events. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1323467