Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons

Details Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..440s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, May-June 1987, p. 440-447. In Russian.

Computer Science

Sound

1

Auroral Zones, Earth Magnetosphere, Polar Regions, Solar Electrons, Current Sheets, High Energy Electrons, Lines Of Force, Satellite Sounding, Time Response

Scientific paper

Intercosmos-17 and ISEE-1 data are used to study the characteristics of the auroral-peak (AP) region: a structure defined by penetrations of high-energy solar electrons on the night side of the polar cap. It is shown that the AP is connected with the precipitation of solar electrons on closed field lines; hence, the penetration boundary of solar electrons on the night side is not the boundary of closed/open flux tubes in the magnetotail. Nonadiabatic scattering of particles in the current sheet is shown to be the most probable mechanism of AP formation.

Affiliated with

Also associated with

No associations

Rating

Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons 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 Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of the structure of the high-latitude magnetosphere according to data on solar electrons will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1817497