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Abstract EGU26-2285 PRIMARY_TEXT retrieval pending

European Geosciences Union · no page hash: the reader saw a rendering, not the bytes · created seq 24186

Link: https://meetingorganizer.copernicus.org/EGU26/EGU26-2285.html · read at 2026-09-29T07:58:00Z · held by reference: only the link, the quoted excerpts with their hashes, and the page hash when the reader had the bytes are stored

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QUOTE {}Its formation requires paleointensity exceeding 11 μT, suggesting a lunar dynamo was active at about 4.2 Ga, as constrained by the superposed basin ejecta.

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