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Magnetic reconnection is an important process in various collisionless plasma environments because it reconfigures the magnetic field and releases magnetic energy to accelerate charged particles. Its dynamics depend critically on the properties of the prereconnection current sheet. One property in particular, cross-sheet temperature inhomogeneity, is ubiquitous throughout the heliosphere. Figure 1 shows an example of such temperature inhomogeneity across the current sheet in Earth’s magnetotail.

astrophysical journal/the astrophysical journal

Energetic Electron Acceleration by Ion-scale Magnetic Islands in Turbulent Magnetic Reconnection: Particle-in-cell Simulations and ARTEMIS Observations