High-Resolution Measurements of the Cross-Shock Potential, Ion Reflection, and Electron Heating at an Interplanetary Shock by MMS

Ian J. Cohen, Steven J. Schwartz, Katherine A. Goodrich, Narges Ahmadi, Robert E. Ergun, Stephen A. Fuselier, Mihir I. Desai, Eric R. Christian, David J. McComas, Gary P. Zank, Jason R. Shuster, Sarah K. Vines, Barry H. Mauk, Robert B. Decker, Brian J. Anderson, Joseph H. Westlake, Olivier Le Contel, Hugo Breuillard, Barbara L. Giles, Roy B. TorbertJames L. Burch

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

The Magnetospheric Multiscale (MMS) spacecraft obtained unprecedented high-time resolution multipoint particle and field measurements of an interplanetary shock event on 8 January 2018. The spacecraft encountered the supercritical forward shock of a forward/reverse shock pair in the pristine solar wind upstream of the bow shock near the subsolar point as they neared apogee at ~25 RE. The high-time resolution measurements from the four spacecraft, separated by only ~20 km, allowed direct measurement of particle distributions revealing evidence of electron heating and near specularly reflected ions. The cross-shock potential is calculated directly from 3-D electric field measurements. This is the first reported direct high temporal resolution (<1 s) observation at an interplanetary shock of near specularly reflected ions. Calculation of the cross-shock potential yields a potential jump significant enough to reflect at least some of the protons from the incident solar wind beam. The cross-shock potential calculated here is consistent with previous estimations based on particle measurements and numerical/analytical simulations. The ambipolar contribution to the cross-shock potential calculated from the four-spacecraft divergence of the electron pressure tensor is somewhat higher than that inferred form the Liouville-mapped electron energy gain across the shock. Furthermore, the high-time-resolution 3-D electric field measurements reported here reveal small-scale nonlinear structures embedded in the shock layer that contribute to the nonmonotonic shock transition.

Original languageEnglish (US)
Pages (from-to)3961-3978
Number of pages18
JournalJournal of Geophysical Research: Space Physics
Volume124
Issue number6
DOIs
StatePublished - Jun 2019

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Keywords

  • MMS
  • interplanetary shock
  • particle acceleration
  • shock potential

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