MMS Observations of Kinetic Alfvén Wave Turbulence and Steep Kinetic-Range Spectra in the Outer Plasma Sheet Boundary Layer

Abstract

Energy dissipation and particle acceleration in the collisionless magnetotail plasma remain incompletely understood. We report observations of Kinetic Alfvén Wave (KAW) turbulence and parallel electric fields ($E_{\parallel }$) in the outer Plasma Sheet Boundary Layer (PSBL) using high-resolution burst-mode data from the Magnetospheric Multiscale (MMS) mission. For a crossing on May 31, 2017, we identify broadband KAW turbulence characterized by a normalized electric-to-magnetic field ratio $\mathcal{R}=|\delta E_{\perp }|/(v_A|\delta B_{\perp }|)=2.5\pm 1.2$ exceeding the MHD limit, a spectral break near ion scales, a steep kinetic-range spectral slope ($\alpha =-3.48\pm 0.13$), and low magnetic compressibility ($C_{\parallel }\approx 0.03$). We observe impulsive $E_{\parallel }$ structures up to 15 mV/m and ion density fluctuations up to 68% during enhanced wave activity. The steep spectrum, compared with undamped KAW predictions ($-7/3$ to $-8/3$), is consistent with substantial energy removal at kinetic scales. The near-zero correlation between the KAW-band filtered $E_{\parallel }$ waveform (0.18 to 2.0 Hz) and ion density fluctuations ($r\approx 0.04$) indicates no simple linear, zero-lag correspondence under the adopted processing. Together with bursty energy-conversion proxies, the observations are consistent with localized field-particle energy exchange and collisionless damping of KAW turbulence in the intermediate-beta outer PSBL. A specific damping channel, such as Landau damping, is not uniquely constrained by the present diagnostics.

20 pages, 6 figures. Published in the Journal of Atmospheric and Solar-Terrestrial Physics