Radial diffusion in Jupiter's magnetosphere

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Electron Diffusion, Electron Energy, Energy Spectra, Jupiter Atmosphere, Planetary Magnetospheres, Radial Flow, Diffusion Coefficient, Nonadiabatic Theory, Pioneer 10 Space Probe, Plasma Turbulence, Whistlers

Scientific paper

Radial phase-space density profiles for equatorially mirroring particles
are computed from data obtained by Pioneer 10. The profiles are
consistent only with radial diffusion subject to nonadiabatic losses. It
is suggested that these losses are due to pitch-angle scattering by
whistler turbulence.

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

Radial diffusion in Jupiter's magnetosphere 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 Radial diffusion in Jupiter's magnetosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial diffusion in Jupiter's magnetosphere will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1570092

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