Explorer 33 entry layer observations

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Magnetohydrodynamic Flow, Magnetopause, Plasma Layers, Satellite Observation, Anisotropy, Boundary Layer Plasmas, Earth Magnetosphere, Explorer 33 Satellite, Magnetic Field Configurations, Magnetosheath, Plasma Diagnostics, Time Dependence

Scientific paper

Low fluxes of stagnant or irregularly flowing plasma along the inside of the magnetopause labeled as the entry layer by Haerendel and Paschmann, are observed on Explorer 33 orbits which cross the dayside magnetopause and on one orbit which skims the dawn flank. The data indicate that the entry layer is a permanent magnetospheric feature which extends across the dayside and along the flanks to large distances down the tail on dipolelike field lines between extensions of the northern and southern polar cusps. Pressure anisotropies are present in the entry layer but are often weaker and less frequent than those in the adjacent magnetosheath. These anisotropies give clues about the process of entry layer formation. The sense of anisotropy when it is present on both sides of the magnetopause is the same for magnetosheath fields with a southward component and opposite for fields with a northward component. These correlations are consistent with entry layer filling by bulk flow along field lines opened by magnetic merging in the one case and by diffusion onto closed field lines in the other.

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

Explorer 33 entry layer 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 Explorer 33 entry layer observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Explorer 33 entry layer observations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-800181

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