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Title: Combined convective and diffusive simulations: VERB-4D comparison with 17 March 2013 Van Allen Probes observations: VERB-4D

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1002/2015GL065230· OSTI ID:1335610
 [1];  [2];  [2];  [3]; ORCiD logo [4];  [5]
  1. Univ. of California, Los Angeles, CA (United States). Dept. of Earth, Planetary, and Space Sciences; Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Dept. of Earth Atmospheric and Planetary Sciences
  2. Univ. of California, Los Angeles, CA (United States). Dept. of Earth, Planetary, and Space Sciences
  3. Univ. of New Hampshire, Durham, NH (United States). Inst. for the Study of Earth, Oceans, and Space
  4. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  5. Univ. of Colorado, Boulder, CO (United States). Lab. of Atmospheric and Space Physics

Our study focused on understanding the coupling between different electron populations in the inner magnetosphere and the various physical processes that determine evolution of electron fluxes at different energies. Observations during the 17 March 2013 storm and simulations with a newly developed Versatile Electron Radiation Belt-4D (VERB-4D) are presented. This analysis of the drift trajectories of the energetic and relativistic electrons shows that electron trajectories at transitional energies with a first invariant on the scale of ~100 MeV/G may resemble ring current or relativistic electron trajectories depending on the level of geomagnetic activity. Simulations with the VERB-4D code including convection, radial diffusion, and energy diffusion are presented. Sensitivity simulations including various physical processes show how different acceleration mechanisms contribute to the energization of energetic electrons at transitional energies. In particular, the range of energies where inward transport is strongly influenced by both convection and radial diffusion are studied. Our results of the 4-D simulations are compared to Van Allen Probes observations at a range of energies including source, seed, and core populations of the energetic and relativistic electrons in the inner magnetosphere.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1335610
Report Number(s):
LA-UR-15-28236
Journal Information:
Geophysical Research Letters, Vol. 42, Issue 22; ISSN 0094-8276
Publisher:
American Geophysical UnionCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 62 works
Citation information provided by
Web of Science

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Cited By (7)

Contemporaneous EMIC and whistler mode waves: Observations and consequences for MeV electron loss: SIMULTANEOUS EMIC AND WHISTLER OBSERVATIONS journal August 2017
Impact of space weather on the satellite industry: Space Weather Impact on Satellites journal June 2017
Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era journal November 2019
Observations and Fokker‐Planck Simulations of the L ‐Shell, Energy, and Pitch Angle Structure of Earth's Electron Radiation Belts During Quiet Times journal February 2019
Multiyear Measurements of Radiation Belt Electrons: Acceleration, Transport, and Loss journal April 2019
Time-Window Approaches to Space-Weather Forecast Metrics: A Solar Wind Case Study journal November 2018
Reanalysis of Ring Current Electron Phase Space Densities Using Van Allen Probe Observations, Convection Model, and Log‐Normal Kalman Filter journal April 2019

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