Quantifying when and where strong magnetic skew forms in a data-driven global non-potential model of the solar corona I: production and persistence of skew.

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Bibliographic Details
Title: Quantifying when and where strong magnetic skew forms in a data-driven global non-potential model of the solar corona I: production and persistence of skew.
Authors: Reid, J1, Mackay, D H1, Upton, L A2
Source: Monthly Notices of the Royal Astronomical Society; Sep2025, Vol. 542 Issue 3, p2184-2210, 27p
Database: Applied Science & Technology Source
Description
ISSN:00358711
DOI:10.1093/mnras/staf1181