The Impact of the Composition on the Properties of Simulated Lunar Mare Basalt Fibers. [PDF]
Liu J +5 more
europepmc +1 more source
Integrative focus on the space exposome-integrome: physiological challenges and practical limits of countermeasures beyond low Earth orbit. [PDF]
Bailey DM +19 more
europepmc +1 more source
Immune Modulation in Cancer: The Role of Tumor-Treating Fields (TTFields). [PDF]
Liu M, Hage ME, Zhao J, Linnebacher M.
europepmc +1 more source
The mediating role of syndecan-4 in the negative association of healthy eating index with body mass index and android percent fat in premenopausal women. [PDF]
Cedillo YE, Moellering DR, De Luca M.
europepmc +1 more source
Relative validity of bioelectrical impedance analysis in estimating body composition in women with overweight and obesity 2 weeks and 6 months postpartum. [PDF]
Westerheim E +5 more
europepmc +1 more source
Polygenic risk for white matter hyperintensities is associated with early cerebrovascular events partly through hemodynamic measures in cognitively unimpaired middle-aged and older adults with low cardiovascular risk. [PDF]
Genius P +12 more
europepmc +1 more source
Lunar Continental Migration and Maria Spreading
Nature, 1970CONTEMPORARY ideas about the broad features of continental migration and ocean floor spreading are largely independent of whether or not there is any sea present. This report considers the possibility that the lunar maria were formed by internal geological processes similar to those which formed the ocean floors of the Earth.
J W Elder
exaly +3 more sources
Lunar maria are not simply large lunar craters. Most craters have raised rims; most maria are bordered partly or wholly by broad zones of downwarping. A satisfactory theory for the origin of maria must provide a genetic link between the origin of the depression and the origin of the material which floors it.
exaly +2 more sources
Thermal instabilities and the formation of lunar maria
The Moon, 1973A model is discussed for a possible type of thermal instability in the outer layers of the Moon. An estimate is made for the temperature differential driving the instability. It is suggested that such an instability may have been involved in the formation of the lunar maria.
J A Bastin
exaly +2 more sources
Lunar Maria: Structure and Evolution
Science, 1969The lunar maria are considered to have evolved as homologous, transient, gravity-wave systems from large impact craters on a crustal layer 50 kilometers thick, fluidized from beneath by prompt, shock-induced melting inside an initially hot moon.
exaly +3 more sources

