Evidence of oblique electron acoustic solitary waves triggered by magnetic reconnection in Earth's magnetosphere
A. Atteya, S. K. EL-Labany, P. K. Karmakar, M. S. Afify

TL;DR
This paper investigates the generation and characteristics of oblique electron acoustic solitary waves in Earth's magnetosphere, revealing how plasma parameters influence wave structures and instability growth, potentially affecting magnetic reconnection processes.
Contribution
It derives a nonlinear Zakharov-Kuznetsov equation for a complex plasma model and analyzes how various parameters influence wave profiles and instability growth rates.
Findings
Wave structures are affected by magnetic field and plasma densities.
Instability growth rate depends on obliquity angle and superthermality.
Enhanced growth rates may lead to increased magnetic reconnection.
Abstract
Motivated by the recent Magnetospheric Multiscale (MMS) observations of oblique electron acoustic waves, we addressed the generation mechanism of the observed waves by utilizing the reductive perturbation technique. The nonlinear Zakharov-Kuznetsov (ZK) equation is derived for collisionless, magnetised plasma composed of cool inertial background electrons, the cool inertial electron beam, hot inertialess suprathermal electrons represented by a -distribution, and stationary ions. Moreover, the instability growth rate is derived by using the small-k perturbation expansion method. Our findings reveal that the structure of the electrostatic wave profile is significantly influenced by the external magnetic field, the unperturbed hot, cool, and electron beam densities, the obliquity angle, and the rate of superthermality. Such parameters also affect the instability growth rate. This…
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Taxonomy
TopicsDust and Plasma Wave Phenomena · Ionosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics
