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Published August 31, 2023 | Version v1
Journal article Open

Possible Lunar Paleointensity Variability During the 3.9 - 3.5 Ga High Field Epoch

Authors/Creators

  • 1. Stanford University

Description

Magnetic hysteresis data, backfield remanence curves, first-order reversal curve (FORC) data, Backscatter Scanning Electron Microscopy (BSEM) images, and specimen name descriptions for the Magnetics Information Consortium (MagIC) that have been utilized in the article titled 'Possible Lunar Paleointensity Variability During the 3.9 - 3.5 Ga High Field Epoch. 

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