Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength

Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength

One of the main theories for heating of the solar corona is based on the idea that solar convection shuffles and tangles magnetic field lines to make many small-scale current sheets that, via reconnection, heat coronal loops. S. K. Tiwari et al. present evidence that, besides depending on loop lengt...

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Bibliographic Details
Main Authors: V. Aparna, Sanjiv K. Tiwari, Ronald L. Moore, Navdeep K. Panesar, Brian Welsch, Bart De Pontieu, Aimee Norton
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar photosphere
Solar magnetic fields
Solar coronal heating
Online Access:https://doi.org/10.3847/1538-4357/add5eb
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