Modeling the Outer Zone Electrons During the July and November 2004 Storms

Details Modeling the Outer Zone Electrons During the July and November 2004 Storms Modeling the Outer Zone Electrons During the July and November 2004 Storms

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsm41c..03b&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM41C-03

Physics

2720 Energetic Particles: Trapped, 2774 Radiation Belts, 2788 Magnetic Storms And Substorms (7954)

Scientific paper

The two largest relativistic electron events of the past solar cycle commenced on 22 July 2004 and on 7 November 2004. Preliminary results modeling electron phase space density at fixed first invariant (2000 MeV/G) throughout both storms using time-dependent radial diffusion coefficients and time-dependent outer boundary conditions were reported last AGU Fall meeting [Brautigam, 2005]. A comparison of final model results to US Air Force CEASE/TSX5 data will be presented. The sensitivity of the results to the various magnetic field models used for computing the adiabatic invariants and how the results relate to the issue of acceleration within the outer boundary will both be discussed. Brautigam, D.H. (2005), Modeling the Relativistic Electron Belt During the July and November 2004 Storms, Eos Trans. 86(52), Fall Meet. Suppl., Abstract SM33A-0435

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