SM019-0006
EDR signatures observed by MMS : a statistical study of dayside events found with machine learning

Thursday, 10 December 2020
Poster
Quentin Lenouvel1, Vincent N Genot2, Philippe Garnier3, Sergio Toledo-Redondo4, Benoit Lavraud5, Nicolas Aunai6, Gautier Nguyen7, Daniel J Gershman8, Robert Ergun9, Per-Arne Lindqvist10, Barbara L Giles8 and James Burch11, (1)IRAP, Toulouse, France, (2)IRAP / CNRS / UPS, PEPS, Toulouse, France, (3)Universite Paul Sabatier, TOULOUSE, France, (4)University of Murcia, Murcia, Spain, (5)IRAP/CNRS, Toulouse, France, (6)Laboratoire de Physique des Plasmas (UMR7648) CNRS/Ecole Polytechnique/UPMC/Univ. Paris Sud/Obs. de Paris Paris (France, Paris, France, (7)Ecole Polytechnique, Palaiseau Cedex, France, (8)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (9)Univ Colorado, Boulder, CO, United States, (10)KTH Royal Institute of Technology, Stockholm, Sweden, (11)Southwest Research Institute, San Antonio, TX, United States
Abstract:
The understanding of magnetic reconnection's physical processes has considerably been improved thanks to the data of the Magnetopsheric Multiscale mission (MMS). However, a lot of work still has to be done to better characterize the core of the reconnection process : the electron diffusion region (EDR). We previously developed a machine learning algorithm to automatically detect EDR candidates, in order to increase the available list of events identified in the literature. However, identifying the parameters that are the most relevant to describe EDRs is complex, all the more that some of the small scale plasma/fields parameters show limitations in some configurations such as for low particle densities or large guide fields cases. In this study, we perform a statistical study of previously reported dayside EDRs as well as newly reported EDR candidates found using machine learning methods. We also show different single and multi-spacecraft parameters that can be used to better identify dayside EDRs in time series from MMS data recorded at the magnetopause.