Work Description

Title: Space Weather Modeling Framework (SWMF) Simulation of Sep 7 2017 Geomagnetic Storm Open Access Deposited

http://creativecommons.org/licenses/by-nc/4.0/
Attribute Value
Methodology
  • This data set contains the outputs of simulations of the geomagnetic storm on Sep 7, 2017 from the Space Weather Modeling Framework (SWMF). Global Ionosphere Thermosphere Model (GITM) was used to simulate the geomagnetic storm on Sep 7, 2017. GITM is driven by high-resolution coupled Block-Adaptive-Tree-Solar Wind-Roe-Upwind-Scheme (BATSRUS) and Rice Convection model (RCM). More details can be found in the paper: Segmentation of Storm Enhanced Density (SED) by Boundary Flows Associated with Partial Ring current, Wang et. al, GRL, 2019
Description
  • SWMF is used to study the segmentation of SED plume into polar cap patches during the geomagnetic storm on Sep 7, 2017. The database includes the 3D output in the upper atmosphere from GITM, the 2D output from Ionospheric Electrodynamics (IE) and 3D output from BATSRUS. The output from GITM can be read with thermo_batch_new.pro. The output from IE can be opened with Spacepy at  https://pythonhosted.org/SpacePy/. The output from BATSRUS can be opened with tecplot. More details can be found in Readme.txt.
Creator
Depositor
  • wzihan@umich.edu
Contact information
Discipline
Funding agency
  • National Science Foundation (NSF)
  • National Aeronautics and Space Administration (NASA)
Keyword
Citations to related material
  • Segmentation of Storm Enhanced Density (SED) by Boundary Flows Associated with Partial Ring current, Wang et. al, GRL, 2019
Resource type
Last modified
  • 08/21/2019
Published
  • 06/14/2019
Language
DOI
License
To Cite this Work:
Wang, Z. (2019). Space Weather Modeling Framework (SWMF) Simulation of Sep 7 2017 Geomagnetic Storm [Data set]. University of Michigan - Deep Blue. https://doi.org/10.7302/9097-z311

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