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Open access Sep 2026

Why a Structureless Solar Corona Is Difficult to Achieve During a Grand Solar Minimum

The structure of the solar corona during the Maunder Minimum (~1645–1715$) remains poorly constrained due to limited direct observations. In spite of this, historical records, including the near-absence of sunspots, reduced auroral activity, elevated cosmogenic isotope levels, and eclipse descriptions, suggest a radica...

P. Riley, R. Caplan, J. Linker et al. · 0 citations

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