EGU25-4690, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-4690
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 10:45–12:30 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X4, X4.109
OpenGGCM simulation of Diamagnetic Cavities in the wake of Flux Transfer Events
Shiva Kavosi
Shiva Kavosi
  • Air Force Research Laboratory, United States of America (kavosi.shiva@gmail.com)

Diamagnetic Cavities (DMCs) characterized by reductions in magnetic field strength and the confinement of proton and electron populations, have been observed in Earth's space environments, including the magnetosheath and magnetosphere. This study focuses on the structure and dynamics of a new type of DMCs generated by Flux Transfer Events (FTEs) within the new region, the low to mid-latitude magnetosphere. Using data from the MMS mission, THEMIS, global MHD simulations, the OpenGGCM model, and particle tracing techniques, we investigate the characteristics, observational signatures, and associated particle energization processes of these "FTE-induced DMCs".  We found that FTE-induced DMC may serve as a new source of high-energy particles in the dayside magnetosphere.

How to cite: Kavosi, S.: OpenGGCM simulation of Diamagnetic Cavities in the wake of Flux Transfer Events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4690, https://doi.org/10.5194/egusphere-egu25-4690, 2025.