ARTEMIS Observations of Plasma Waves in Laminar and Perturbed Interplanetary Shocks
L. Davis, C.A. Cattell, L.B. Wilson III, Z.A. Cohen, A.W. Breneman,, E.L.M. Hanson

TL;DR
This study uses ARTEMIS spacecraft data to analyze plasma wave properties in interplanetary shocks, revealing differences in wave activity and energy dissipation between laminar and perturbed shocks.
Contribution
It provides the first detailed comparison of plasma wave characteristics in laminar versus perturbed interplanetary shocks using ARTEMIS data.
Findings
Laminar shocks show higher wave activity in the transition region.
Perturbed shocks exhibit fewer large amplitude waves in the ramp.
Energy dissipation via wave-particle interactions is greater in laminar shocks.
Abstract
The 'Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun' (ARTEMIS) mission provides a unique opportunity to study the structure of interplanetary shocks and the associated generation of plasma waves with frequencies between ~50-8000 Hz due to its long duration electric and magnetic field burst waveform captures. We compare wave properties and occurrence rates at 11 quasi-perpendicular interplanetary shocks with burst data within 10 minutes (~3200 proton gyroradii upstream, ~1900 downstream) of the shock ramp. A perturbed shock is defined as possessing a large amplitude whistler precursor in the quasi-static magnetic field with an amplitude greater than 1/3 the difference between the upstream and downstream average magnetic field magnitudes; laminar shocks lack these large precursors and have a smooth, step function-like transition. In…
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