Publication Date:
2017-11-01
Description:
We use theory and simulations to study how the out-of-plane (guide) magnetic field strength modifies the location where the energy conversion rate between the electric field and the plasma is appreciable during asymmetric magnetic reconnection, motivated by observations (Genestreti et al. , this issue). For weak guide fields, energy conversion is maximum on the magnetospheric side of the X-line, midway between the X-line and electron stagnation point. As the guide field increases, the electron stagnation point gets closer to the X-line, and energy conversion occurs closer to the electron stagnation point. We motivate one possible non-rigorous approach to extend the theory of the stagnation point location to include a guide field. The predictions are compared to two-dimensional particle-in-cell (PIC) simulations with vastly different guide fields. The simulations have upstream parameters corresponding to three events observed with MMS. The predictions agree reasonably well with the simulation results, capturing trends with the guide field. The theory correctly predicts that the X-line and stagnation points approach each other as the guide field increases. The results are compared to MMS observations, Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE) observations of each event, and a global resistive magnetohydrodynamics simulation of the 2015 Oct 16 event. The PIC simulation results agree well with the global observations and simulation, but differ in the strong electric fields and energy conversion rates found in MMS observations. The observational, theoretical, and numerical results suggest that the strong electric fields observed by MMS do not represent a steady global reconnection rate.
Print ISSN:
0148-0227
Topics:
Geosciences
,
Physics
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