Inner Radiation Belt Data Assimilation

Details Inner Radiation Belt Data Assimilation Inner Radiation Belt Data Assimilation

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm33c1927g&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM33C-1927

Physics

[2720] Magnetospheric Physics / Energetic Particles: Trapped, [2774] Magnetospheric Physics / Radiation Belts

Scientific paper

We present preliminary results of inner belt proton data assimilation using an augmented version of the Selesnick et al., [2007] model. The physics-based model computes inner belt proton intensities as a function of time and of the three adiabatic invariants M, K, and L according to a comprehensive list of inner belt source and loss processes. We modify the model solution based on in-situ proton observations and according to a data-assimilation method which exploits the non-Gaussian nature of inner belt proton intensities and Poisson or Gaussian counting statistics of the observations, as appropriate. We demonstrate the method by presenting data-assimilated inner belt proton intensities during a solar particle injection.

Affiliated with

Also associated with

No associations

Rating

Inner Radiation Belt Data Assimilation 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 Inner Radiation Belt Data Assimilation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inner Radiation Belt Data Assimilation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1471573