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Fig. 5 | Earth, Planets and Space

Fig. 5

From: The problem of the acceleration of electrons of the outer radiation belt and magnetospheric substorms

Fig. 5

Plasma 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)

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