Abstract
AbstractWe develop an algorithm that finds a trajectory through simulations of magnetic reconnection along which input Magnetospheric Multiscale (MMS) spacecraft observations are matched. Using two‐dimensional particle‐in‐cell simulations of asymmetric reconnection, the method is applied to a magnetopause electron diffusion region (EDR) encountered by the MMS spacecraft to facilitate interpretation of the event based on fully kinetic models. The recently discovered crescent‐shaped electron velocity distributions measured by MMS in the EDR are consistent with simulation distributions at the corresponding time along the computed trajectory.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.