Energy transfer and conversion in magnetic reconnection: Observation and simulation
One of the central problems in collisionless plasma turbulence is to understand the nature of the cross-scale energy transfer and dissipation occurring at kinetic scales. Magnetic reconnection plays an important role in dissipating energy and driving energy transfer in these systems. However, for reconnection, a detailed picture of the fluxes of energy in its several forms, and the conversion among them, until now remains unclear. In this study, a scale filtering method is adopted to explore how energy is converted between different forms and transferred across scales in turbulent magnetic reconnection using a combination of Magnetospheric Multiscale observations and particle-in-cell simulations. Two novel findings of this paper are that both ion and electron dissipation start to occur at sub-ion scale, at nearly same scale, and that most of the energy cascade due to reconnection is carried by the electron fluid.
Authors
- Sohom Roy (ORCID: https://orcid.org/0000-0003-3891-5495)
- W. H. Matthaeus (ORCID: https://orcid.org/0000-0001-7224-6024)
- R. Bandyopadhyay (ORCID: https://orcid.org/0000-0002-6962-0959)
- Subash Adhikari (ORCID: https://orcid.org/0000-0003-2160-7066)
- Yan Yang (ORCID: https://orcid.org/0000-0003-2965-7906)
Institutions
- Princeton University (US)
- University of Delaware (US)
Publication Details
- Journal
- Physics of Plasmas
- Published
- 2025-11-01
- DOI
- https://doi.org/10.1063/5.0278907
- Primary Topic
- Ionosphere and magnetosphere dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Science Foundation
- National Aeronautics and Space Administration
- Princeton University
- Nuclear Safety and Security Commission