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Turbulent Energy Transfer at Dipolarization Fronts
被引:5
|作者:
Liu, C. M.
[1
,2
]
Cao, J. B.
[1
,2
]
Xing, X. N.
[1
,2
]
Chen, Z. Z.
[3
]
机构:
[1] Beihang Univ, Sch Space & Environm, Beijing, Peoples R China
[2] Minist Ind & Informat Technol, Key Lab Space Environm Monitoring & Informat Proc, Beijing, Peoples R China
[3] Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Res Lab PEARL, Zhuhai, Peoples R China
基金:
中国国家自然科学基金;
关键词:
energy transfer;
dipolarization fronts;
waves;
turbulence;
BURSTY BULK FLOWS;
PARTICLE-ACCELERATION;
KINETIC-ANALYSIS;
PLASMA;
CONVERSION;
TRANSPORT;
FIELD;
D O I:
10.1029/2023GL104185
中图分类号:
P [天文学、地球科学];
学科分类号:
07 ;
摘要:
Dipolarization fronts (DFs), ion-scale magnetic transients characterized by dramatic enhancement of northward magnetic field, have been documented as crucial energy transfer regions in the magnetosphere. DF-driven energy transfer has hitherto been studied mainly in the laminar regime. Energy transfer driven by turbulent processes, however, remains unclear. Here we perform a comprehensive investigation of turbulent energy transfer (TET) developed at DFs, via using high-cadence data from Magnetospheric Multiscale mission. We find that: (a) TET is equally governed by energy loads and generators, different from laminar energy transfer which is typically dominated by energy loads; (b) ion and electron currents play comparable roles in driving TET; (c) TET is positively correlated with local magnetic field strength and ion speed; (d) TET shows asymmetric global distributions along the dawn-dusk direction. These features implicate that TET is primarily related to electromagnetic turbulence at electron-ion hybrid scales. These new results, uncovering unique characteristics of DF-driven TET, can deeply advance our understanding of energy budgets in the magnetosphere.
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页数:10
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