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Crustal structure of the Moon determined from short-period Rayleigh wave analysis

The lunar crustal structure is determined to be in a depth range of 0 to 40 km by means of Rayleigh wave analysis. The traces of three moonquakes were used to obtain Rayleigh wave dispersion (group velocities) in the short period range (fundamental mode: 0.5–12.5 s, first mode: 0.5–5.5 s, and second...

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I tiakina i:
Ngā taipitopito rārangi puna kōrero
Kaituhi matua: Victor Corchete
Hōputu: Artigo
Reo:Inglês
I whakaputaina: Frontiers Media S.A. 2025-05-01
Rangatū:Frontiers in Astronomy and Space Sciences
Ngā marau:
Urunga tuihono:https://www.frontiersin.org/articles/10.3389/fspas.2025.1433697/full
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