In this section
@article{Madanian:2020:10.1002/essoar.10503047.1,
author = {Madanian, H and Schwartz, SJ and Halekas, JS and Wilson, LB},
doi = {10.1002/essoar.10503047.1},
title = {Nonstationary Quasi-perpendicular Shock and Ion Reflection at Mars},
url = {http://dx.doi.org/10.1002/essoar.10503047.1},
year = {2020}
}
TY - JOUR
AB - <jats:p>Collisionless shocks in space plasma are regions of heating andacceleration of charged particles and dissipation of kinetic energy.These accelerated particles are the source of electromagnetic emissionsfrom supernova remnants and other astrophysical structures. At high Machnumbers, shocks can be inherently nonstationary and exhibit modulatedenergy transfer and recurring plasma compression areas in the form ofreformation. We use data from the Mars Atmosphere and Volatile Evolution(MAVEN) spacecraft to study reformation of the Martian bow shock whichhas a relatively high curvature compared to that at Earth and theupstream solar wind is often mass loaded with a population of pickupions. We show evidence of ion reflection effects in reformation of asupercritical quasi-perpendicular shock.</jats:p>
AU - Madanian,H
AU - Schwartz,SJ
AU - Halekas,JS
AU - Wilson,LB
DO - 10.1002/essoar.10503047.1
PY - 2020///
TI - Nonstationary Quasi-perpendicular Shock and Ion Reflection at Mars
UR - http://dx.doi.org/10.1002/essoar.10503047.1
UR - https://doi.org/10.1002/essoar.10503047.1
ER -