We utilize a theoretical analysis of the generation, ascent, intrusion and eruption of basaltic
magma on the Moon to develop new insights into magma source depths, supply processes …

This work provides an introduction to the foundations of three-dimensional c-puter vision
and describes recent contributions to the? eld, which are of methodical and application …

To understand the dynamics of shallow magmatic intrusions, I propose a theoretical model
of magma spreading laterally below an elastic crust. Nondimensionalization of the flow …

Mare Fecunditatis is a~ 310,000 km2 flat basalt plain located in the low-latitude area of the
Moon. Plenty of volcanic features (multiple episodes of mare basalts, sinuous rilles, lava …

Mons Rümker is a large volcanic complex in Oceanus Procellarum on the Moon and is a
candidate landing site for China's Chang'E‐5 sample return mission. We conducted a …

The morphology and topography of volcanic landforms provide critical information to the
investigation of their tectonic setting and the physical characteristics (eg, rheology) of their …

The volcanic style of the Moon has long been understood to consist almost exclusively of
flood basalts erupted from fissures along with minor pyroclastic activity; large central vent …

Mare domes, small shield volcanoes typically<∼ 30 km diameter, are part of the spectrum of
lunar volcanic features that characterize extrusive basalt deposits. We used new spacecraft …

The Gruithuisen domes, situated on the western portion of the Imbrium basin rim, form three
tall mountains (NW, Gamma, Delta) totaling∼ 780 km 3 in volume. The shapes of the domes …

Volcanism is an important geological evolutionary process on the Moon. The study of lunar
volcanic features is of great significance and value to understanding the geological …