Calculation of Field-line Slippage Rates in Coronal Simulations

Abstract We present the universal Slippage calculator ( USlip ), an extension of the universal Fieldline Tracer ( UFiT ), which computes magnetic field line slippage rates from an input magnetic field defined on a structured grid. The slippage rate provides a local, physically grounded diagnostic of nonideal evolution, directly quantifying departures from ideal frozen-in motion. We outline the theoretical formulation and describe an efficient numerical implementation. The method is validated against analytical solutions and applied to simulations using three coronal codes treating varying spatial scales, all of which are standard inputs for USlip . In all the examples considered, the slippage rate not only identifies where magnetic connectivity changes occur but also accurately reproduces the observed direction of field-line slippage. The consistency of the results across analytical tests and multiple simulation platforms demonstrates that USlip is a robust and versatile tool for diagnosing 3D reconnection in dynamically evolving systems.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-09-09
DOI
https://doi.org/10.3847/1538-4357/ae9948
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Calculation of Field-line Slippage Rates in Coronal Simulations

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Calculation of Field-line Slippage Rates in Coronal Simulations

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article en

Abstract

Abstract We present the universal Slippage calculator ( USlip ), an extension of the universal Fieldline Tracer ( UFiT ), which computes magnetic field line slippage rates from an input magnetic field defined on a structured grid. The slippage rate provides a local, physically grounded diagnostic of nonideal evolution, directly quantifying departures from ideal frozen-in motion. We outline the theoretical formulation and describe an efficient numerical implementation. The method is validated against analytical solutions and applied to simulations using three coronal codes treating varying spatial scales, all of which are standard inputs for USlip . In all the examples considered, the slippage rate not only identifies where magnetic connectivity changes occur but also accurately reproduces the observed direction of field-line slippage. The consistency of the results across analytical tests and multiple simulation platforms demonstrates that USlip is a robust and versatile tool for diagnosing 3D reconnection in dynamically evolving systems.

The Astrophysical JournalVol. 1008(2)
University of Dundee (GB), Durham University (GB), University of Trento (IT), Montana State University (US), University of Michigan (US), University of Glasgow (GB)
National Science Foundation, National Aeronautics and Space Administration, UK Research and Innovation, Leverhulme Trust, University of Cambridge, Science and Technology Facilities Council
Climate action
Openalex Percentile: Top 17%
Solar and Space Plasma Dynamics
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