Lunar mare basalt flow units: Thicknesses determined from crater size‐frequency distributions
- 27 April 2002
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 29 (8), 89-1-89-4
- https://doi.org/10.1029/2002gl014847
Abstract
No abstract availableThis publication has 10 references indexed in Scilit:
- Ages of mare basalts on the lunar nearsideJournal of Geophysical Research, 2000
- Characteristics of lunar mare deposits in Smythii and Marginis basins: Implications for magma transport mechanismsJournal of Geophysical Research, 1998
- Volumes of lunar lava ponds in South Pole‐Aitken and Orientale Basins: Implications for eruption conditions, transport mechanisms, and magma source regionsJournal of Geophysical Research, 1997
- Lunar mare volcanism: Stratigraphy, eruption conditions, and the evolution of secondary crustsGeochimica et Cosmochimica Acta, 1992
- Lava flooding of ancient planetary crusts: Geometry, thickness, and volumes of flooded lunar impact basinsEarth, Moon, and Planets, 1982
- Thicknesses of lunar mare flow frontsEarth, Moon, and Planets, 1981
- Geometric interpretation of lunar cratersProfessional Paper, 1980
- Lunar volcanism in space and timeReviews of Geophysics, 1976
- Effects of lava flows on lunar crater populationsEarth, Moon, and Planets, 1976
- Thicknesses of some lunar mare basalt flows and ejecta blankets based on chemical kinetic dataGeochimica et Cosmochimica Acta, 1975