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- W2952357504 abstract "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 R E . 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." @default.
- W2952357504 created "2019-06-27" @default.
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- W2952357504 date "2019-06-01" @default.
- W2952357504 modified "2023-10-10" @default.
- W2952357504 title "High‐Resolution Measurements of the Cross‐Shock Potential, Ion Reflection, and Electron Heating at an Interplanetary Shock by MMS" @default.
- W2952357504 cites W1487280089 @default.
- W2952357504 cites W1550765676 @default.
- W2952357504 cites W1578289780 @default.
- W2952357504 cites W1581159005 @default.
- W2952357504 cites W1608574704 @default.
- W2952357504 cites W1619856765 @default.
- W2952357504 cites W1628830896 @default.
- W2952357504 cites W1630828591 @default.
- W2952357504 cites W1654924962 @default.
- W2952357504 cites W1960790191 @default.
- W2952357504 cites W1966244157 @default.
- W2952357504 cites W1968507639 @default.
- W2952357504 cites W1972314626 @default.
- W2952357504 cites W1973197582 @default.
- W2952357504 cites W1974840361 @default.
- W2952357504 cites W1979489455 @default.
- W2952357504 cites W1984063221 @default.
- W2952357504 cites W1984756998 @default.
- W2952357504 cites W1987170112 @default.
- W2952357504 cites W1993734459 @default.
- W2952357504 cites W1997244919 @default.
- W2952357504 cites W1997790639 @default.
- W2952357504 cites W1998223744 @default.
- W2952357504 cites W2004410789 @default.
- W2952357504 cites W2009947728 @default.
- W2952357504 cites W2012385392 @default.
- W2952357504 cites W2022719771 @default.
- W2952357504 cites W2030885661 @default.
- W2952357504 cites W2032807998 @default.
- W2952357504 cites W2036650128 @default.
- W2952357504 cites W2042251717 @default.
- W2952357504 cites W2046538186 @default.
- W2952357504 cites W2052947135 @default.
- W2952357504 cites W2053570386 @default.
- W2952357504 cites W2054113022 @default.
- W2952357504 cites W2063286394 @default.
- W2952357504 cites W2064821532 @default.
- W2952357504 cites W2069942517 @default.
- W2952357504 cites W2070505416 @default.
- W2952357504 cites W2072359146 @default.
- W2952357504 cites W2075101167 @default.
- W2952357504 cites W2075425556 @default.
- W2952357504 cites W2077151048 @default.
- W2952357504 cites W2079414711 @default.
- W2952357504 cites W2081907750 @default.
- W2952357504 cites W2082449559 @default.
- W2952357504 cites W2082486808 @default.
- W2952357504 cites W2083029054 @default.
- W2952357504 cites W2085914529 @default.
- W2952357504 cites W2087815660 @default.
- W2952357504 cites W2101636949 @default.
- W2952357504 cites W2113004519 @default.
- W2952357504 cites W2113303802 @default.
- W2952357504 cites W2118126719 @default.
- W2952357504 cites W2121307982 @default.
- W2952357504 cites W2122877469 @default.
- W2952357504 cites W2131531891 @default.
- W2952357504 cites W2139626991 @default.
- W2952357504 cites W2148043627 @default.
- W2952357504 cites W2149670948 @default.
- W2952357504 cites W2151921276 @default.
- W2952357504 cites W2153255288 @default.
- W2952357504 cites W2153543644 @default.
- W2952357504 cites W2170138653 @default.
- W2952357504 cites W2172143247 @default.
- W2952357504 cites W2201603632 @default.
- W2952357504 cites W2321480352 @default.
- W2952357504 cites W2337440446 @default.
- W2952357504 cites W2417614483 @default.
- W2952357504 cites W2742326052 @default.
- W2952357504 cites W2749904267 @default.
- W2952357504 cites W2806526068 @default.