Browsing Physics by Author "Wang, X"

Now showing items 1-10 of 10

Global Hybrid Simulations of Interaction Between Interplanetary Rotational Discontinuity and Bow Shock/Magnetosphere: Can Ion-Scale Magnetic Reconnection be Driven by Rotational Discontinuity Downstream of Quasi-Parallel Shock?

Guo, Zhifang; Lin, Yu; Wang, X; 0000-0002-3728-6319 (2022-09-29)

Ion-scale magnetic reconnection has been observed downstream of the terrestrial quasi-parallel (Q-parallel to) shock. Whether it is driven by interplanetary discontinuities or turbulent Q-parallel to shock, however, is ...

Global-scale hybrid simulation of cusp precipitating ions associated with magnetopause reconnection under southward IMF

Tan, B; Lin, Y; Perez, J; Wang, X (2022-09-20)

With a 3-D global-scale hybrid simulation model, we investigate the energy spectra of cusp precipitating ions and issues associated with magnetopause reconnection under a southward IMF. Both the spatial and temporal energy ...

Global-scale hybrid simulation of dayside magnetic reconnection under southward IMF: Structure and evolution of reconnection

Tan, B; Lin, Y; Perez, J; Wang, X (2022-09-20)

Magnetopause reconnection is investigated with our 3-D self-consistent global hybrid simulation model. The magnetic configuration and evolution of Flux Transfer Events (FTEs) and the associated ion density and ion velocity ...

Hall effect control of magnetotail dawn-dusk asymmetry: A three-dimensional global hybrid simulation

Lu, San; Lin, Y.; Angelopoulos, V; Artemyev, A; Pritchett, P; Lu, Quanming; Wang, X; 0000-0003-3041-2682; 0000-0003-2085-1171 (2022-10-27)

Magnetotail reconnection and related phenomena (e.g., flux ropes, dipolarizing flux bundles, flow bursts, and particle injections) occur more frequently on the duskside than on the dawnside. Because this asymmetry can ...

Hybrid simulation of foreshock waves and ion spectra and their linkage to cusp energetic ions

Wang, X; Lin, Y; Chang, S (2022-10-25)

A three-dimensional global hybrid simulation is carried out to investigate energetic ions and electromagnetic waves in the quasi-parallel (Q-parallel to) bow shock and cusp for a typical interplanetary magnetic field ...

Investigation of storm timemagnetotail and ion injection using three-dimensional global hybrid simulation

Lin, Y; Wang, X; Lu, S; Perez, J; Lu, Q (2022-09-29)

Dynamics of the near-Earth magnetotail associated with substorms during a period of extended southward interplanetary magnetic field is studied using a three-dimensional (3-D) global hybrid simulation model that includes ...

The ion temperature gradient: An intrinsic property of Earth's magnetotail

Lu, San; Artemyev, A; Angelopoulos, V; Lin, Y; Wang, X (2022-11-01)

Although the ion temperature gradient along (X-GSM) and across (Z(GSM)) the Earth's magnetotail, which plays a key role in generating the cross-tail current and establishing pressure balance with the lobes, has been ...

Magnetotail-Inner Magnetosphere Transport Associated With Fast Flows Based on Combined Global-Hybrid and CIMI Simulation

Lin, Y; Wang, X; Fok, M; Buzulukova, N; Perez, J; Cheng, L; Chen, L; 0000-0002-4768-189X; 0000-0002-5619-9093; 0000-0002-8127-2248 (2022-11-01)

Using the combined Auburn global hybrid simulation code in 3-D (ANGIE3D) and the Comprehensive Inner Magnetosphere-Ionosphere (CIMI) model, we investigate the self-consistent connection of fast flow injections from the ...

Three-dimensional global hybrid simulation of dayside dynamics associated with the quasi-parallel bow shock

Lin, Yu; Wang, X (2022-09-29)

A three-dimensional global-scale hybrid simulation is carried out, for the first time, for dynamics of the dayside bow shock-magnetosphere system associated with the quasi-parallel bow shock. A case with IMF along the ...

Three-dimensional hybrid simulation of magnetosheath reconnection under northward and southward interplanetary magnetic field

Pang, Y; Lin, Y; Deng, X; Wang, X; Tan, B (2022-09-29)

A three-dimensional (3-D) global hybrid simulation is carried out for the generation and structure of magnetic reconnection in the magnetosheath because of the interaction of an interplanetary tangential discontinuity (TD) ...