Cold ion effects in density-asymmetric collisionless magnetic reconnection

被引:0
|
作者
Sun, Mengmeng [1 ]
Mao, Aohua [1 ,2 ,3 ]
He, Xianglei [1 ]
Divin, Andrey [4 ]
Zou, Jitong [1 ]
Wang, Zhibin [5 ]
Zhou, Tianchun [1 ]
Wang, Xiaogang [1 ,2 ,3 ]
机构
[1] Harbin Inst Technol, Sch Phys, Harbin 150001, Peoples R China
[2] Harbin Inst Technol, Lab Space Environm & Phys Sci, Harbin 150001, Peoples R China
[3] Harbin Inst Technol, China Russia Belt & Rd Joint Lab Adv Energy & Powe, Harbin 150001, Peoples R China
[4] St Petersburg State Univ, Dept Earths Phys, St Petersburg 198504, Russia
[5] Sun Yat Sen Univ, Sino French Inst Nucl Engn & Technol, Zhuhai 519082, Peoples R China
基金
俄罗斯科学基金会; 中国国家自然科学基金;
关键词
magnetic reconnection; cold ions; particle-in-cell (PIC); asymmetric density; particle distribution functions; MAGNETOPAUSE;
D O I
10.1088/1361-6587/ad670b
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The coexistence of low-energy (cold) ions and thermal (warm) ions is commonly observed in space and laboratory plasmas, such as those in magnetopause and fusion fueling processes. In certain events, the cold ion proportion may play a crucial role in plasma processes, especially magnetic reconnection. In this paper, magnetic reconnection with density-asymmetric cold ions is investigated in implicit particle-in-cell (iPIC) simulations. It is found that in such events the reconnection rate decreases as the cold ion distribution depth into the current sheet increases, mainly due to the mass-loading effect. Particularly, a density-peak structure of cold ions is developed in the reconnection region owing to the bounce motion of cold ions entering from the opposite inflow region. In the y-vy phase space where the y-direction is normal to the current sheet, a cold ion ring structure related to the bounce motion is formed and amplified by the Hall electric field. Furthermore, the cold ions become a notable current carrier due to its shorter inertial scale than the warm ions. Consequently, the asymmetry of the cold ion distribution significantly breaks the symmetry in the Hall magnetic field, eventually leading to asymmetric cold ion density peak structure. Such structures can be taken as significant signals of cold ion existence in in situ spacecraft observations.
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页数:13
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