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Electron behaviour around the onset of magnetic reconnection
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  • Susanne Flø Spinnangr,
  • Michael Hesse,
  • Paul Tenfjord,
  • Cecilia Norgren,
  • Håkon Midthun Kolstø,
  • Norah Kaggwa Kwagala,
  • Therese Moretto Jørgensen,
  • Tai D Phan
Susanne Flø Spinnangr
Space Plasma Physics Group, Department of Physics and Technology, University of Bergen

Corresponding Author:[email protected]

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Michael Hesse
NASA Ames Research Center
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Paul Tenfjord
University of Bergen
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Cecilia Norgren
Department of Physics and Technology, University of Bergen
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Håkon Midthun Kolstø
Space Plasma Physics Group, University of Bergen
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Norah Kaggwa Kwagala
University of Bergen
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Therese Moretto Jørgensen
NASA Ames Research Center
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Tai D Phan
Space Sciences Laboratory, University of California Berkeley
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Abstract

We investigate the onset of magnetic reconnection, utilizing a fully kinetic Particle-In-Cell (PIC) simulation. Characteristic features of the electron phase-space distributions immediately before reconnection onset are identified. These include signatures of pressure non-gyrotropy in the velocity distributions, and lemon shaped distributions in the in-plane velocity directions. Further, we explain how these features form through particle energization by the out-of-plane electric field. Identification of these features in the distributions can aid in analysis of data where clear signatures of ongoing reconnection are not yet present.