MHD-test particles simulations of moderate CME and CIR-driven geomagnetic storms at solar minimum
Authors/Creators
- 1. Dartmouth College, NCAR High Altitude Observatory
- 2. Laboratory for Atmospheric and Space Physics, University of Colorado Boulder
- 3. Dartmouth College
- 4. NCAR High Altitude Observatory
- 5. The Aerospace Corporation
- 6. University of Iowa
Description
field100x180.t0.data contains results from GAMERA code to produce Figure 3. Variables, grids, and units are described in the file.
May2019_kp3_2000_both-Lstar_PSD.h5 contains simulated 2000 MeV/G electron phase space density during the May event on a radial and time grid and is used to plot Figure 5. Its radial profile at 05/14 10UT is used in Figure 7a. The unit of PSD is (c/MeV/cm)^3.
May2019_kp3_5000_both-Lstar_PSD.h5 contains simulated 5000 MeV/G electron phase space density during the May event on a radial and time grid. Its radial profile at 05/14 10UT is used in Figure 7b. The unit of PSD is (c/MeV/cm)^3.
Sept2019_Gamera_2000_both-Lstar_PSD.h5 contains simulated 2000 MeV/G electron phase space density during the May event on a radial and time grid and is used to plot Figure 6. Its radial profile at 09/03 00UT is used in Figure 7c. The unit of PSD is (c/MeV/cm)^3.
Sept2019_Gamera_5000_both-Lstar_PSD.h5 contains simulated 5000 MeV/G electron phase space density during the May event on a radial and time grid. Its radial profile at 09/03 00UT is used in Figure 7d. The unit of PSD is (c/MeV/cm)^3.