Search Publications

Electron acceleration in the near-Earth magnetotail: test particle calculations in electromagnetic fields from two-dimensional hybrid simulations
DOI: 10.1007/s10509-017-3093-0 Bibcode: 2017Ap&SS.362..119G

Wu, Mingyu; Du, Aimin; Guo, Zhifang

Electron acceleration in the near-Earth magnetotail during the substorm period is still an unresolved question. In this paper, by tracing electron trajectories in the dynamically evolving electromagnetic fields obtained from a two-dimensional (2D) global hybrid simulation, we investigate electron acceleration in the near-Earth magnetotail during d…

2017 Astrophysics and Space Science
Cluster 4
Double-cusp simulation during northward IMF using 3D PIC global code
DOI: 10.1007/s10509-017-3098-8 Bibcode: 2017Ap&SS.362..125E

Esmaeili, Amin; Kalaee, Mohammad Javad

The cusp has important effects on the transportation of particles and their energy from the solar wind to the magnetosphere, and ionosphere, and high-altitude atmosphere. The cusp can be considered to be a part of the magnetospheric boundary layer with weaker magnetic fields. It has been studied since 1971 by different satellite observations. Desp…

2017 Astrophysics and Space Science
Cluster 3
Nonlinear evolution of oblique whistler waves in radiation belts
DOI: 10.1007/s10509-016-3003-x Bibcode: 2017Ap&SS.362...32S

Sharma, R. P.; Sharma, Swati; Nandal, P. +1 more

Magnetic power spectrum and formation of coherent structures have been investigated in the present work applicable to Van Allen radiation belt. The nonlinear interaction of high frequency oblique whistler wave and low frequency magnetosonic wave has been investigated. Simulation was performed of the coupled equation of these two waves. The nonline…

2017 Astrophysics and Space Science
Cluster 0
Energy budget during an isolated substorm using measurements of multi satellites and geomagnetic indices
DOI: 10.1007/s10509-017-3072-5 Bibcode: 2017Ap&SS.362..101M

Dunlop, M. W.; Ma, Yuduan; Yang, Jian +1 more

Measurements of multi satellites and geomagnetic indices are used to investigate the energy budget during an isolated substorm. The calculation of the energy transfer from the solar wind to the magnetosphere (parameter ɛ), the energy increase of the ring current (

2017 Astrophysics and Space Science
Cluster 0