Abstract
AbstractWe employ a 2.5D particle‐in‐cell simulation to study a scenario where the reconnection process captures cold streaming protons. As soon as the tailward streaming protons become involved, they contribute to the overall momentum balance, altering the initially symmetric dynamics. Adding tailward‐directed momentum to the reconnection process results in a tailward propagation of the reconnection site. We investigate how the reconnection process reorganizes itself due to the changing momentum conditions on the kinetic scale and how the reconnection rate is affected. We find that adding tailward momentum does not result in a significantly different reconnection rate compared to the case without cold streaming protons, when scaled to the total Alfvén velocity. This implies that the effect of changing inflow conditions due to the motion of the reconnection site appears to be minimal. The dynamics of the particles are, however, significantly different depending on whether they enter on the tailward or Earthward side of the reconnection site. On the Earthward side they are reflected and thermalized, while on the tailward side they are picked up and accelerated. The cold proton density and Ez on the Earthward side are turbulent, while the tailward side has laminar cold proton density striations and an embedded Ez layer. Also, since the initial plasma sheet population is swept up on one side and flushed out on the other, asymmetries in the densities and strength of Hall fields emerge. Our results are important for understanding the development and dynamics of magnetospheric substorms and storms.
Highlights
Magnetic reconnection describes the process facilitating the release of stored electromagnetic energy into mechanical energy of the plasma, producing a global change of the magnetic configuration due to local decoupling of plasma from the magnetic field
We find that adding tailward momentum does not result in a significantly different reconnection rate compared to the case without cold streaming protons, when scaled to the total Alfvén velocity
These clear density striations in the tailward exhaust are a signature that the cold streaming protons are confined and that the vertical distance corresponds to their meandering width
Summary
Magnetic reconnection describes the process facilitating the release of stored electromagnetic energy into mechanical (kinetic and thermal) energy of the plasma, producing a global change of the magnetic configuration due to local decoupling of plasma from the magnetic field. The effect of ions originating from the ring current and warm plasma cloak has been observed not to greatly affect the reconnection rate (Fuselier et al, 2016; Wang et al, 2015) Another source of heavy ions on the dayside is O+ originating from the high-latitude ionosphere. Since the Larmor radius depends on the mass and velocity, these different ion populations will lead to a different kinetic behavior and additional scale lengths in the system (Alm et al, 2019; André et al, 2016; Dargent et al, 2019; Divin et al, 2016; Toledo-Redondo et al, 2015) In this manuscript we study how a streaming population is captured by the reconnection process and what the effects are.
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