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. 2017 Sep 9;44(17):8712–8720. doi: 10.1002/2017GL074895

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©2017. The Authors.

This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

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(a) Satellite locations at ~13:20 on 14 December 2015. (b, first panel) Btotal on VAP‐A (−80 nT) in blue, on MMS1 in green, and on GOES‐13 (−35 nT) in purple. Note that the rapid change seen on MMS at ~13:25 is a crossing into the magnetosheath and back into the magnetosphere. (b, second panel) E _y on MMS1. (b, third panel) E _y on VAP‐A (spin period resolution due to loss of one spherical probe). (b, fourth panel) E _y on on VAP‐B. (b, fifth panel) solar wind pressure (purple) and SYM‐H (divided by 10, black).