Final published version
Licence: CC BY: Creative Commons Attribution 4.0 International License
Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
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TY - JOUR
T1 - Evidence of Alfvénic Activity in Jupiter's Mid‐To‐High Latitude Magnetosphere
AU - Lorch, C. T. S.
AU - Ray, L. C.
AU - Wilson, R. J.
AU - Bagenal, F.
AU - Crary, F.
AU - Delamere, P. A.
AU - Damiano, P. A.
AU - Watt, C. E. J.
AU - Allegrini, F.
PY - 2022/6/30
Y1 - 2022/6/30
N2 - Abstract: Using a combination of Juno magnetometer and plasma data, we show evidence of Alfvénic turbulence within the mid‐to‐high latitude magnetosphere with sufficient conditions to trigger auroral particle acceleration. We analyze 12 events that, in agreement with theoretical results, are found to be dissipative at the electron inertial scale. Furthermore, these events contain significant Poynting flux in the range ∼0.8–20 mW/m2 at ionospheric altitudes. This is sufficient to generate auroral emissions. We confirm that such events are incompressible, confirming their Alfvénicity, occur at dissipative scales, have intermittent features present and are multifractal in nature. These results illustrate the importance of turbulence in the mid‐to‐high latitudes of Jupiter's magnetosphere as a driver of particle acceleration.
AB - Abstract: Using a combination of Juno magnetometer and plasma data, we show evidence of Alfvénic turbulence within the mid‐to‐high latitude magnetosphere with sufficient conditions to trigger auroral particle acceleration. We analyze 12 events that, in agreement with theoretical results, are found to be dissipative at the electron inertial scale. Furthermore, these events contain significant Poynting flux in the range ∼0.8–20 mW/m2 at ionospheric altitudes. This is sufficient to generate auroral emissions. We confirm that such events are incompressible, confirming their Alfvénicity, occur at dissipative scales, have intermittent features present and are multifractal in nature. These results illustrate the importance of turbulence in the mid‐to‐high latitudes of Jupiter's magnetosphere as a driver of particle acceleration.
KW - Magnetospheric Physics
KW - IONOSPHERE
KW - Ionosphere/magnetosphere interactions
KW - Particle acceleration
KW - Wave/particle interactions
KW - MAGNETOSPHERIC PHYSICS
KW - Magnetosphere/ionosphere interactions
KW - Planetary magnetospheres
KW - PLANETARY SCIENCES: SOLID SURFACE PLANETS
KW - Magnetospheres
KW - PLANETARY SCIENCES: FLUID PLANETS
KW - PLANETARY SCIENCES: COMETS AND SMALL BODIES
KW - RADIO SCIENCE
KW - Waves in plasma
KW - SPACE PLASMA PHYSICS
KW - Research Article
KW - Jupiter
KW - Alfven
KW - turbulence
KW - electron
KW - energization
KW - magnetosphere
U2 - 10.1029/2021ja029853
DO - 10.1029/2021ja029853
M3 - Journal article
VL - 127
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
SN - 2169-9402
IS - 6
M1 - e2021JA029853
ER -