Inverse energy dispersion of energetic ions observed in the magnetosheath

We thank the FGM, FPI, and EPD instrument teams of MMS mission and ARTEMIS mission for the successful spacecraft operation and for providing plasma and magnetic field data. This research was supported by an appointment to the NASA Postdoctoral Program appointment at the NASA/GSFC, administered by Universities Space Research Association through a contract with NASA. Some of the work conducted at NASA/GSFC was supported by the MMS project. J.M.R. acknowledges the support of NSF under AGS-1341918. M.L. is supported by NERC grant NE/K011766/1. The SuperDARN radars are funded by the national scientific agencies of Australia, Canada, China, France, Japan, South Africa, United Kingdom, and the United States. We thank the team of Katie Herlingshaw, Suzie Imber, Hammed Lawal, Tim Yeoman, Jasmine Sandhu, Rosie Johnson, and Timothy David at the University of Leicester who collected the Hankasalmi radar data used in this paper which supported the CAPER rocket campaign. We thank the national institutes that support them and INTERMAGNET for promoting high standards of magnetic observatory practice. We also thank E. Yizengaw, E. Zesta, M.B. Moldwin, and the rest of the AMBER team for the data. AMBER is operated by Boston College and funded by NASA and AFOSR.