Published January 23, 2022 | Version v2

SWMF/CIMI outputs used in Holappa and Buzulukova (2022) manuscript submitted to Geophys. Res. Lett.

  • 1. University of Oulu
  • 2. NASA GSFC

Description

These data files and Python scripts are used to produce Figures 1 and 2 in Holappa and Buzulukova, Explicit IMF By-dependence of energetic protons and the ring current, submitted to Geophys. Res. Lett. (2022).

PARAM.in.PosTilt and gitinfo.txt contain the settings and Git version references used to setup the SWMF model.

Figure 1: PosBy_CimiFlux_n00000046_h.fls, NegBy_CimiFlux_n00000046_h.fls are CIMI output files containing proton fluxes for different energies and pitch angles. These data can be read with CIMIreader.py. Figures in the manuscript can be produced by Run_CIMI_reader.py. Files PosBy_CimiFlux_n00000046_e.fls, NegBy_CimiFlux_n00000046_e.fls can be used to produce corresponding figures for electrons.

Figure 2: Data files CIMI_log_NegBy_PosTilt.dat and  CIMI_log_PosBy_PosTilt.dat are CIMI output files containing the ring current energy and other variables. Figures can be produced by Plot_CIMI_Dst.py. 

 

Files

gitinfo.txt

Files (487.4 MB)

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Additional details

Funding

Research Council of Finland
Explaining a new solar wind driver of geomagnetic activity 322459