Diamagnetic Suppression of Component Magnetic Reconnection at the Magnetopause
M. Swisdak, B. N. Rogers, J. F. Drake, M. A. Shay
Abstract
We present particle-in-cell simulations of collisionless magnetic reconnection in a system (like the magnetopause) with a large density asymmetry across the current layer. In the presence of an ambient component of the magnetic field perpendicular to the reconnection plane the gradient creates a diamagnetic drift that advects the X-line with the electron diamagnetic velocity. When the relative drift between the ions and electrons is of the order the Alfven speed the large scale outflows from the X-line necessary for fast reconnection cannot develop and the reconnection is suppressed. We discuss how these effects vary with both the plasma beta and the shear angle of the reconnecting field and discuss observational evidence for diamagnetic stabilization at the magnetopause.
Create a lesson
Related papers
The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024
Maxime Grandin, Emma Bruus, Vincent E. Ledvina et al.
Validation of Space Weather Forecasting at Leonid Space
Scott Shambaugh
Data-driven prediction of atomic-oxygen erosion yield in polymers from bulk physical properties
Youngwoo Choi, Doeun Koo, Seungbum Hong et al.
What Caused the Orbital Decay of the Twin Van Allen Probes to Diverge?
Ayisha M Ashruf, Ankush Bhaskar, C Vineeth et al.
A Student Sounding Rocket Experiment to Probe Electron Density in the Lower Ionosphere
Joshua Goodwill, Timothy Tomaszewski, Jarrod Bieber et al.
Revisiting magnetotelluric theory: layered induction and geoelectric fields
Dennies Bor