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

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 w...

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Veröffentlicht in:Journal of geophysical research. Space physics 2019-06, Vol.124 (6), p.3961-3978
Hauptverfasser: Cohen, Ian J., Schwartz, Steven J., Goodrich, Katherine A., Ahmadi, Narges, Ergun, Robert E., Fuselier, Stephen A., Desai, Mihir I., Christian, Eric R., McComas, David J., Zank, Gary P., Shuster, Jason R., Vines, Sarah K., Mauk, Barry H., Decker, Robert B., Anderson, Brian J., Westlake, Joseph H., Le Contel, Olivier, Breuillard, Hugo, Giles, Barbara L., Torbert, Roy B., Burch, James L.
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Sprache:eng
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Zusammenfassung: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 (
ISSN:2169-9380
2169-9402
DOI:10.1029/2018JA026197