Articles | Volume 39, issue 6
https://doi.org/10.5194/angeo-39-991-2021
https://doi.org/10.5194/angeo-39-991-2021
Regular paper
 | 
06 Dec 2021
Regular paper |  | 06 Dec 2021

Magnetotail reconnection asymmetries in an ion-scale, Earth-like magnetosphere

Christopher M. Bard and John C. Dorelli

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Latest update: 11 Dec 2024
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Short summary
We use a computer code to study how a particular plasma effect, the Hall effect, changes how plasma behaves and interacts with magnetic fields behind planets in the magnetotail. We find that when the scale of the Hall effect is big enough compared to the scale of the magnetotail, plasma behavior is no longer symmetric. Measurements of magnetic activity and structure vary in time and differ between opposite sides of the tail. This fits well with findings from spacecraft data and other models.