Other
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsm11a1167l&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SM11A-1167
Other
7827 Kinetic And Mhd Theory, 2740 Magnetospheric Configuration And Dynamics, 2744 Magnetotail, 2748 Magnetotail Boundary Layers, 2764 Plasma Sheet
Scientific paper
During geomagnetically active periods, magnetic field fluctuations are frequently observed. We present Cluster ion observations obtained in the near-Earth magnetotail from 15 to 20 Re. When field fluctuations are prominent, ion distributions become irregular. In particular, holes appear in ion velocity space distributions in the tailward direction. On the other hand, ions moving in the Earthward direction are accelerated and form beam-like distributions. The holes in velocity space are gyrophase dependent and suggest a sink of particles nearby the spacecraft. The directions of ion holes and beam-like distributions are quite steady even though magnetic field direction is changing. This results in high anisotropy in V⊥, which yields large velocity moments perpendicular to the magnetic field. The presence of large ∂ B/B suggests that a temporal mechanism (for example, scattering by waves) plays a role in the formation of the gyrophase-dependent holes and beam-like distributions. Possible mechamisms responsible for these observations will be investigated.
Bavassano-Catanneo M.-
Bosqued J.
Dandouras Iannis
Fillingim M.
Kistler Lynn
No associations
LandOfFree
Observations of ion velocity space holes associated with magnetic field fluctuations in the plasma sheet 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 Observations of ion velocity space holes associated with magnetic field fluctuations in the plasma sheet, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of ion velocity space holes associated with magnetic field fluctuations in the plasma sheet will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1463807