Phase-space contributions to pressure and stress tensors in the electron diffusion region of magnetic reconnection
Magnetic reconnection is a fundamental plasma process in collisionless plasma that governs the transfer of magnetic energy to plasma energy through a change in magnetic topology. The reconnection electric field, or equivalently, the rate at which the magnetic flux is reconnected, must everywhere satisfy momentum balance. In this study, using in situ spacecraft measurements from the Magnetospheric MultiScale mission, supported by test-particle simulations and kinetic particle-in-cell simulations, we investigate how various electron populations contribute to the reconnection electric field inside the electron diffusion region by supplying or diverting momentum away from the X line. We show that the electron pressure anisotropy that develops in the inflow reduces the reconnection electric field by transporting momentum toward the X line. A net outward flux of momentum in the direction normal to the current sheet likely contributes positively to the reconnection electric field.
Authors
- D. B. Graham (ORCID: https://orcid.org/0000-0002-1046-746X)
- M. Hesse (ORCID: https://orcid.org/0000-0003-0377-9673)
- Y. V. Khotyaintsev (ORCID: https://orcid.org/0000-0001-5550-3113)
- T. D. Phan (ORCID: https://orcid.org/0000-0002-6924-9408)
- C. Norgren (ORCID: https://orcid.org/0000-0002-6561-2337)
- Norah Kaggwa Kwagala (ORCID: https://orcid.org/0000-0003-4789-8084)
Institutions
- Uppsala University (SE)
- Ames Research Center (US)
- Swedish Institute of Space Physics (SE)
- University of Bergen (NO)
- University of California, Berkeley (US)
Publication Details
- Journal
- Physics of Plasmas
- Published
- 2025-05-01
- DOI
- https://doi.org/10.1063/5.0246402
- Citations
- 3
- Primary Topic
- Ionosphere and magnetosphere dynamics
- Type
- article
- Field-Weighted Citation Impact
- 3.46
Funders
- Swedish National Space Agency
- Knut och Alice Wallenbergs Stiftelse
- Norges Forskningsråd