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.
引用
收藏
页数:10
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