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Updated: Jun 21, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability

Magnetically Induced Rotating Rayleigh-Taylor Instability

Published on: March 3, 2017

Collisionless magnetic reconnection via Alfvén eigenmodes.

¹School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA.

Physical Review Letters

|August 8, 2009

Summary

This summary is machine-generated.

This study introduces an analytic approach to collisionless magnetic reconnection, viewing it as Alfvén eigenmode generation and dissipation. The findings align with in situ measurements of Hall fields during reconnection events.

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Published on: July 20, 2022

Area of Science:

Plasma Physics
Astrophysics
Space Physics

Background:

Collisionless magnetic reconnection is a fundamental process in plasma physics.
Understanding its dynamics is crucial for space weather and astrophysical phenomena.

Purpose of the Study:

To develop an analytic approach for collisionless magnetic reconnection.
To model reconnection as Alfvén eigenmode generation and dissipation.

Main Methods:

Formulating reconnection as Alfvén eigenmode dynamics.
Confining eigenmodes within a current sheet, analogous to quantum mechanical wave confinement.
Calculating the dynamical time scale using the n=1 mode eigenvalue propagation velocity.

Main Results:

The dynamical time scale of reconnection is determined by the system scale and the n=1 mode velocity.
The analytic prediction for the n=1 mode shows good agreement with in situ measurements.
Hall fields associated with reconnection are accurately predicted by the model.

Conclusions:

Alfvén eigenmodes provide a viable framework for understanding collisionless magnetic reconnection.
The proposed analytic model accurately captures key aspects of reconnection dynamics, including Hall field generation.