Turbulence in Magnetic Reconnection Jets from Injection to Sub-Ion Scales

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Richard, L., Sorriso-Valvo, L., Yordanova, E., Graham, D. B., Khotyaintsev, Yu. V.
Format: Preprint
Publié: 2023
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866911767079157760
author Richard, L.
Sorriso-Valvo, L.
Yordanova, E.
Graham, D. B.
Khotyaintsev, Yu. V.
author_facet Richard, L.
Sorriso-Valvo, L.
Yordanova, E.
Graham, D. B.
Khotyaintsev, Yu. V.
contents We investigate turbulence in magnetic reconnection jets in the Earth's magnetotail using data from the Magnetospheric Multiscale spacecraft. We show that signatures of a limited inertial range are observed in many reconnection jets. The observed turbulence develops on the time scale of a few ion gyroperiods, resulting in intermittent multifractal energy cascade from the characteristic scale of the jet down to the ion scales. We show that at sub-ion scales, the fluctuations are close to mono-fractal and predominantly kinetic Alfvén waves. The observed energy transfer rate across the inertial range is $\sim 10^8~\mathrm{J}~\mathrm{kg}^{-1}~\mathrm{s}^{-1}$, which is the largest reported for space plasmas so far.
format Preprint
id arxiv_https___arxiv_org_abs_2303_08693
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Turbulence in Magnetic Reconnection Jets from Injection to Sub-Ion Scales
Richard, L.
Sorriso-Valvo, L.
Yordanova, E.
Graham, D. B.
Khotyaintsev, Yu. V.
Space Physics
Plasma Physics
We investigate turbulence in magnetic reconnection jets in the Earth's magnetotail using data from the Magnetospheric Multiscale spacecraft. We show that signatures of a limited inertial range are observed in many reconnection jets. The observed turbulence develops on the time scale of a few ion gyroperiods, resulting in intermittent multifractal energy cascade from the characteristic scale of the jet down to the ion scales. We show that at sub-ion scales, the fluctuations are close to mono-fractal and predominantly kinetic Alfvén waves. The observed energy transfer rate across the inertial range is $\sim 10^8~\mathrm{J}~\mathrm{kg}^{-1}~\mathrm{s}^{-1}$, which is the largest reported for space plasmas so far.
title Turbulence in Magnetic Reconnection Jets from Injection to Sub-Ion Scales
topic Space Physics
Plasma Physics
url https://arxiv.org/abs/2303.08693