Published September 14, 2020 | Version v2
Dataset Open

Coupling the Rice Convection Model-Equilibrium to the Lyon– Fedder–Mobarry Global Magnetohydrodynamic Model

Authors/Creators

  • 1. Rice University
  • 2. Rice Unviersity
  • 3. SUST
  • 4. NCAR

Contributors

Contact person:

  • 1. Rice University

Description

Self-consistent inner-magnetosphere model is driven by inputs from the Lyon-Fedder- Mobarry global magnetohydrodynamic model.

The expanded inner magnotospheric modeling region captures high-resolution bursty bulk flows in the plasma sheet.

Realistic bursty bulk flows induced aurora patterns are simulated.

This includes data and visualization methods that reproduce the figures in the manuscript. Please refer to README for details.

Submitted to JGR for review. 

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Bao_et_al_JGR_2020.zip

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