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IMPTAM electron distributions

Equatorial maps

1-10 keV10-50 keV
e0 e1
50-100 keV100-500 keV
e2 e3

Radial map spectrograms

0h MLT12h MLT
spectr_mlt_0 spectr_mlt_12
6h MLT18h MLT
spectr_mlt_6 spectr_mlt_18

MLT pitch angle distributions

0h MLT12h MLT
pad_mlt_0 pad_mlt_12

IMPTAM homepage.

Key model publications

  • Ganushkina N. Yu., O. Amariutei, Y. Y. Shpritz, and M. Liemohn (2013), Transport of the plasma sheet electrons to the geostationary distances, J. Geophys. Res., 118, doi:10.1029/2012JA017923.
  • Ganushkina N. Yu., M. Liemohn, O. Amariutei, and D. Pitchford (2014), Low energy electrons (5-50 keV) in the inner magnetosphere, J. Geophys. Res., 119, 246-259, doi:10.1002/2013JA019304.
  • Ganushkina N. Yu., O. A. Amariutei, D. Welling, and D. Heynderickx, (2015), Nowcast model for low-energy electrons in the inner magnetosphere, Space Weather, 13, doi:10.1002/2014SW001098.
  • Ganushkina N. (2022), Operational inner magnetosphere particle transport and acceleration model (IMPTAM) for 1–300 keV electron, Adv. Sp. Res. In press, doi 10.1016/j.asr.2022.10.022.