SH042-0002
A Statistical MMS Survey of Properties and Origin of Electrostatic Solitary Waves in Quasi-perpendicular Earth's Bow Shocks

Tuesday, 15 December 2020
Poster
Rachel Wang1, Ivan Vasko2, Stuart Bale3, Forrest Mozer3 and Anton Artemyev4, (1)University of California Berkeley, Berkeley, CA, United States, (2)Space Science Lab, UC berkeley, Moscow, CA, United States, (3)University of California, Berkeley, Berkeley, CA, United States, (4)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States
Abstract:
We performed a statistical analysis of more than 1200 electrostatic bipolar structures measured by Magnetospheric Multiscale spacecrafts in 9 quasi-perpendicular Earth’s bow shock crossings, ranging in amplitude from 10 mV/m up to 800 mV/m. The bipolar structures propagate highly oblique to the shock normal with velocities on the order of ion-acoustic velocity and have spatial scales of a few Debye lengths. Through interferometry analysis, we find that the majority of the bipolar structures have negative electrostatic potentials, and about 3% have positive potentials. Our analysis leads to the interpretation that negative potential structures are ion phase space holes produced by ion two-stream instability between incoming and reflected ions near the ramp of the shock, while positive potential structures are either electron holes or ion-acoustic solitons with the latter interpretation being more plausible. We present a summary of the physical natures of bipolar structures and discuss how these results are in agreement with this theory on their generation mechanism.