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Lunar mare basalt flow units: Thicknesses determined from crater size-frequency distributions

Published:2002-04 Issue:8 Volume:29 Page:89-1-89-4
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Hiesinger H.¹,Head J. W.¹,Wolf U.²,Jaumann R.²,Neukum G.²

Affiliation:

1. Department of Geological Sciences; Brown University; Providence RI USA

2. DLR - Inst. of Space Sensor Technology and Planetary Exploration; Berlin Germany

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference23 articles.

1. Thicknesses of some lunar mare basalt flows and ejecta blankets based on chemical kinetic data;Brett;Geochim. Cosmochim. Acta,1975

2. Thickness of mare material in the Tranquillitatis and Nectaris basins;DeHon;Proc. Lunar Planet. Sci. Conf.,1974

3. Thickness of the western mare basalts;DeHon;Proc. Lunar Planet. Sci. Conf.,1979

4. Geologic structure of the eastern mare basins;DeHon;Proc. Lunar Planet. Sci. Conf.,1976

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4. Volcanic thermal demagnetization of the Reiner Gamma magnetic anomaly;Icarus;2023-10

5. Determining the thermal histories of Apollo 15 mare basalts using diffusion modelling in olivine;Geochimica et Cosmochimica Acta;2023-09

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