# Three-Dimensional X-line Spreading in Asymmetric Magnetic Reconnection

## TL;DR

This study uses 3D particle-in-cell simulations to explore how the X-line spreads in asymmetric magnetic reconnection, revealing a dependence on current sheet thickness and identifying conditions for Alfvénic spreading.

## Contribution

It demonstrates that X-line spreading speed depends on current sheet thickness and reconnection conditions, highlighting the role of kinetic Alfvén waves and tearing instability in the process.

## Key findings

- X-line spreads at ion/electron drift speeds in thick sheets.
- Alfvénic spreading occurs in thinner sheets with faster propagation.
- Simulation results align with magnetopause observations.

## Abstract

The spreading of the X-line out of the reconnection plane under a strong guide field is investigated using large-scale three-dimensional (3D) particle-in-cell (PIC) simulations in asymmetric magnetic reconnection. A simulation with a thick, ion-scale equilibrium current sheet (CS) reveals that the X-line spreads at the ambient ion/electron drift speeds, significantly slower than the Alfv\'en speed based on the guide field $V_{Ag}$. Additional simulations with a thinner, sub-ion-scale CS show that the X-line spreads at $V_{Ag}$ (Alfv\'enic spreading), much higher than the ambient species drifts. An Alfv\'enic signal consistent with kinetic Alfv\'en waves develops and propagates, leading to CS thinning and extending, which then results in reconnection onset. The continuous onset of reconnection in the signal propagation direction manifests as Alfv\'enic X-line spreading. The strong dependence on the CS thickness of the spreading speeds, and the X-line orientation are consistent with the collisionless tearing instability. Our simulations indicate that when the collisionless tearing growth is sufficiently strong in a thinner CS such that $\gamma/\Omega_{ci}\gtrsim\mathcal{O}(1)$, Alfv\'enic X-line spreading can take place. Our results compare favorably with a number of numerical simulations and recent magnetopause observations. A key implications is that the magnetopause CS is typically too thick for Alfv\'enic X-line spreading to effectively take place.