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Abstract EGU26-2285 PRIMARY_TEXT

European Geosciences Union · no page hash: the reader saw a rendering, not the bytes · created seq 24034

Link: https://meetingorganizer.copernicus.org/EGU26/EGU26-2285.html · read at 2026-09-29T02:51:01Z · 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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FETCHED at 2026-09-29T05:09:35Z · https://meetingorganizer.copernicus.org/EGU26/EGU26-2285.html · seq 25454

Server hash sha256:9a398f3627309ae10cf0ca0ac3fb0d87b1298dfd41d520d9491d0bd838d3ab22 · 164610 bytes · text/html. The reader's record is unchanged; this is the server's finding beside it.

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We identify a shallow, magnetized, high-density body consistent with buried mare basalt. Its formation requires paleointensity exceeding 11 μT, suggesting a ...not found — this server looked at the page and did not find the passage

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QUOTE {}We identify a shallow, magnetized, high-density body consistent with buried mare basalt. Its formation requires paleointensity exceeding 11 μT, suggesting a lunar dynamo was active at about 4.2 Ga, as constrained by the superposed basin ...

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