the National Natural Science Founda-tion of China(NSFC,Grant No.42174181)and the Key Research Program of Frontier Sciences,CAS(Grant No.QYZDJ-SSW-DQC010).
The formation of an embedded electron current sheet within the magnetotail plasma sheet has been poorly understood.In this article,we present an electron current layer detected at the edge of the magnetotail plasma sh...
The 3D simulation was carried out by the K computer at the RIKEN Advanced Institute for Computational Science through the HPCI Research project(hp140129,hp150123);supported by the National Natural Science Foundation of China under Grant Nos.42350710793,41874189 and 41821003。
A recent satellite observation has revealed the presence of energy conversion in the separatrix region(SR)of magnetotail reconnection,driven by perpendicular components.We investigated this phenomenon by means of part...
supported by NSFC grants(42188101,42174209,42174207);the Specialized Research Fund for State Key Laboratories of China;the Strategic Pioneer Program on Space Science II,Chinese Academy of Sciences,grants XDA15350201,XDA15052500.
Based on current sheet flapping motion on 27 August 2018 in the dusk flank magnetotail,as recorded by instruments aboard Magnetospheric Multiscale(MMS)spacecraft,we present the first study of guide field reconnection ...
the National Natural Science Foundation of China(42030101,42204158);Shanghai Pujiang Program(No.21PJD078);Shanghai Science and Technology Innovation Action Plan(No.21DZ1206100);the Fundamental Research Funds for the Central Universities.
Magnetosonic waves are an important medium for energy transfer in collisionless space plasma.Magnetosonic waves have been widely investigated in the upstream of the bow shock at Mars.These waves are believed to origin...
supported by the National Natural Science Foundation of China (grants 42025404, 42188101, 41904144, and 41674163);the preresearch projects on Civil Aerospace Technologies (grants D020303, D020104, and D020308);funded by the China National Space Administration;the B-type Strategic Priority Program of the Chinese Academy of Sciences (grant XDB41000000);the Fundamental Research Funds for the Central Universities (grants 2042021kf1045 and 2042021kf1056)
Tailward ion outflows in the Martian-induced magnetotail are known to be one of the major channels for Martian atmospheric escape.On the basis of nearly 6.5 years of observations from the Mars Atmosphere and Volatile ...
the National Natural Science Foundation of China(41174144,40974098)。
In this paper,the y-component of magnetic field line curvature in the plasma sheet was analyzed,and two kinds of shear structures of the flapping current sheet were found,i.e.symmetric and antisymmetric.The alternatin...
The ion-to-electron temperature ratio is a good indicator of the processes involved in solar wind plasma entering and being transported inside Earth’s plasma sheet.In this study,we have demonstrated that patchy magne...
supported by the National Natural Science Foundation of China(NSFC)under grants 41731070,41674167,41574161;the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences,grants XDA15052500,XDA15350201 and XDA15011401;the Specialized Research Fund for State Key Laboratories of China.
With conjunction observations of electromagnetic fields and plasma from Time History of Events and Macroscale Interactions during Substorm(THEMIS)in the near-Earth magnetotail,we investigate the spatial and temporal p...
This work was supported by the pre-research projects on Civil Aerospace Technologies funded by China’s National Space Administration(CNSA)(Grant No.D020103);and the National Natural Science Foundation of China(Grant Nos.41474144,41674176).
It has been confirmed that dipolarization fronts(DFs)are the result of the interchange instability in the Earth's magnetotail.In this paper,we use a Hall MHD model to simulate the evolution of the interchange instabil...
supported by the National Natural Science Foundation of China (Grant Nos. 41404133, 41874188, 41574153, 40621003 & 41431071);supported by the project (Grant No. KP19-270);Christine GABRIELSE was supported by NASA (Grant No. NAS5-02099);the support by NASA’s MMS project at Sw RI and NSF (Grant Nos. AGS1602510, NASA NNX16AI39G/80NSSC18K1534, 80NSSC18K0570 & 80NSSC18K0693)
In this paper, the particle acceleration processes around magnetotail dipolarization fronts(DFs) were reviewed. We summarize the spacecraft observations(including Cluster, THEMIS, MMS) and numerical simulations(includ...