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Published January 23, 2022 | Version v1

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).

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

Files (487.3 MB)

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md5:2d058f0bf3c5e9fe3a586ab2d46c83da
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md5:03da64bb7b9fdbf671805a8b0537d183
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Additional details

Funding

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