Evaluation of energetic particle parameters in the near-Earth magnetotail derived from flux asymmetry observations

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4

Scientific paper

The flux asymmetries measured by spectrometers on board spacecraft contain information on particle parameters. The net flux intensity (NFI) method provides a tool to evaluate these parameters. The NFI method is valid when both the spin period of the spacecraft and the time resolution of the particle spectrometers are much shorter than the characteristic time-scale of the particle flux variations. We apply the NFI analysis to the flux asymmetry measurements made by GEOS 2 at the nightside geosynchronous orbit in the late substorm growth phase. The cross-tail current of energetic ions, their pressure gradient and average drift velocity, as well as a field-aligned flows are investigated. Current disruption at substorm onset and the convection surge mechanism during dipolarization of the magnetic field are directly observed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Evaluation of energetic particle parameters in the near-Earth magnetotail derived from flux asymmetry observations 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 Evaluation of energetic particle parameters in the near-Earth magnetotail derived from flux asymmetry observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaluation of energetic particle parameters in the near-Earth magnetotail derived from flux asymmetry observations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1656354

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.