Substorm plasma sheet ion pressure profiles

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2724 Magnetopause And Boundary Layers, 2736 Magnetosphere/Ionosphere Interactions (2431), 2744 Magnetotail, 2764 Plasma Sheet, 2790 Substorms

Scientific paper

The plasma sheet pressure, temperature, and density profiles inferred from DMSP observations are used to investigate substorm growth, expansion, early-recovery, and late-recovery phases. During the growth phase, the pressure peaks at the inner edge of the plasma sheet. The premidnight pressure peak is associated with the temperature peak, while the postmidnight peak is associated with the density enhancement. After the substorm onset, the pressure at the inner edge diminishes. Instead, the pressure peaks at premidnight from X = -10 to -40 RE, which can be associated with temperature enhancement. During the early and late recovery phases, the pressure peaks at postmidnight, which is associated with a cold, dense ion population, possibly resulting from ion outflow and the substorm current systems. In the near-Earth region, the entropy decreases after substorm onset, but the specific entropy appears to be roughly conserved.

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

Substorm plasma sheet ion pressure profiles 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 Substorm plasma sheet ion pressure profiles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Substorm plasma sheet ion pressure profiles will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1420848

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