Fig. 5From: The problem of the acceleration of electrons of the outer radiation belt and magnetospheric substormsPlasma pressure profiles obtained from the DMSP data shown in Fig. 2. Plasma pressure profiles obtained from the DMSP F17 satellite data during the auroral crossing on 8 October 2012 between 21:47:40 and 21:52:50 UT mapped to the equatorial plane by IGRF (red) and Tsyganenko 2004 (blue) models, we used the methodology proposed by Stepanova et al. (2004, 2006, 2008)Back to article page