A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results

Details A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh43a1934w&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH43A-1934

Physics

Plasma Physics

[2124] Interplanetary Physics / Heliopause And Solar Wind Termination, [2126] Interplanetary Physics / Heliosphere/Interstellar Medium Interactions, [7833] Space Plasma Physics / Mathematical And Numerical Techniques

Scientific paper

We present a model for determining neutral particle distributions in astrospheres. In a general numeric method we are not restricted to Maxwellian velocity distributions. Results pertaining to the modification of Kappa distributions due to gravitational forces and ionization losses are demonstrated. Energetic Neutral Atom (ENA) instruments have made the conceptual leap of moving from an in-situ particle sensor to a remote sensing observation. We compare the various approaches of simulating the neutral particle environment for this leap, using IBEX data as a proving ground.

Affiliated with

Also associated with

No associations

Rating

A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results 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 A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Kinetic Reverse Trajectory Model for Space Neutral Particle Simulations - Heliospheric Results will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-879586