EGU25-2163, updated on 25 Mar 2025
https://doi.org/10.5194/egusphere-egu25-2163
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 28 Apr, 14:00–14:10 (CEST)
 
Room 1.14
Plasma dynamics in the diffusion regions of magnetic reconnection
Cecilia Norgren1 and the ISSI MMS Workshop Team*
Cecilia Norgren and the ISSI MMS Workshop Team
  • 1Swedish Institute of Space Physics, Uppsala, Sweden (cecilia.norgren@irfu.se)
  • *A full list of authors appears at the end of the abstract

Magnetic reconnection is a fundamental plasma process responsible for the sometimes explosive release of magnetic energy in space and laboratory plasmas. Inside the diffusion regions of magnetic reconnection, the plasma becomes demagnetized and decouples from the magnetic field, enabling the change in magnetic topology necessary to power the energy release over larger scales. Since it was launched in 2015, the Magnetospheric MultiScale (MMS) mission has significantly advanced the understanding of the particle dynamics key to magnetic reconnection by providing high-resolution, in-situ measurements able to resolve ion and electron kinetic scales that have confirmed theoretical predictions, revealed new phenomena, and refined existing models. These breakthroughs are critical for understanding not only space plasmas but also laboratory and astrophysical plasmas where magnetic reconnection occurs. In this talk, we give a brief review and present some recent results of selected topics related to the ion and electron dynamics occurring within the diffusion regions.  

ISSI MMS Workshop Team:

'Magnetic Reconnection: Explosive Energy Conversion in Space Plasmas'

How to cite: Norgren, C. and the ISSI MMS Workshop Team: Plasma dynamics in the diffusion regions of magnetic reconnection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2163, https://doi.org/10.5194/egusphere-egu25-2163, 2025.