Snapshot View of 3D Reconnection Simulation at late time @nasamms
Snapshot View of 3D Reconnection Simulation at late time  @nasamms
Uploaded February 2011 | Updated September 2026, 2 weeks ago
Inside box: isosurface of current density colored by the particle density.
Side panels: color coded current density.
Guide field is present at 50% of inflow field intensity. The electron current sheet that is produced during the development of reconnection is breaking up into filaments in 3D, and this leads to the creation of "flux ropes" in which the magnetic field lines begin to wrap around the current filaments.
After Daughton et al., 2011 Nature Physics, TBD.
Snapshot View of 3D Reconnection Simulation at late timeWhat scientific questions was MMS designed to explore in the magnetosphere?Principal Investigator - The MMS MissionMMS Hot Plasma Composition AnalyzerLocation and Data Collection System - Chuck CoteIntro to magnetic reconnection - How is energy released during magnetic reconnection?Intro to magnetic reconnection - How do coronal mass ejections (CMEs) affect material in space?Education and Public Outreach Mission Lead - The MMS MissionRecycle your office paperIntro to magnetic fields - How does magnetic field strength vary with distance?The Oceans and our Changing Climate - Jeremy WerdellSolarium Demo
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Snapshot View of 3D Reconnection Simulation at late time

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