Physics
Scientific paper
Feb 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ssrv...91..507n&link_type=abstract
Space Science Reviews, v. 91, Issue 3/4, p. 507-577 (2000).
Physics
11
Scientific paper
Geomagnetic field lines that are stretched on the nightside of the Earth due to reconnection with the interplanetary magnetic field constitute the Earth's magnetotail. The magnetotail is a dynamic entity where energy imparted from the solar wind is stored and then released to generate disturbance phenomena such as substorms. This paper gives an updated overview on the physics of the magnetotail by drawing heavily from recent research conducted with the GEOTAIL satellite. It summarizes firstly the basic properties of the magnetotail such as shape, size and magnetic flux content, internal motion and plasma regimes. Then it describes characteristics of tail plasmas of the solar-wind and the ionosphere origins. Thirdly it addresses acceleration and heating of plasmas in the magnetotail, where reconnection between the stretched field lines is the main driver but the site of the acceleration is not limited to the immediate vicinity of the neutral line. In the collisionless regime of the plasma sheet kinetic behaviors of ions and electrons control the acceleration process. The paper closes by enumerating the problems posed for future studies.
Nishida Akira
No associations
LandOfFree
The Earth's Dynamic Magnetotail 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 The Earth's Dynamic Magnetotail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Earth's Dynamic Magnetotail will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1714457