Results 311 to 320 of about 164,975 (347)
Environmental health risk assessment and acute effects of sulfur dioxide (SO2) inhalation exposure on traditional sulfur miners at Ijen Crater Volcano, Indonesia. [PDF]
Susetyo SH+4 more
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Control and Modelling of Laser Shock Peening without Coating (LSPwC) Texture of AISI 9310 Steel. [PDF]
Liu P, Yang Z, Xie C, Yang F, Zhou L.
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Dichotomy retreat and aqueous alteration on Noachian Mars recorded in highland remnants. [PDF]
McNeil JD+5 more
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▪ Abstract The detailed morphology of impact craters is now believed to be mainly caused by the collapse of a geometrically simple, bowl-shaped “transient crater.” The transient crater forms immediately after the impact. In small craters, those less than approximately 15 km diameter on the Moon, the steepest part of the rim collapses into the crater ...
Boris A. Ivanov, H. J. Melosh
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The biology of impact craters — a review
Biological Reviews, 2002ABSTRACTImpact craters contain ecosystems that are often very different from the ecosystems that surround them. On Earth over 150 impact craters have been identified in a wide diversity of biomes. All natural events that can cause localized disruption of ecosystems have quite distinct patterns of recovery.
Cockell, Charles S., Lee, Pascal
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Elements, 2012
Impact cratering is an important and unique geologic process. The high speeds, forces and temperatures involved are quite unlike conventional endogenic processes, and the environmental consequences can be catastrophic. Kilometre-scale craters are excavated and collapse in minutes, in some cases distributing debris around the globe and exhuming deeply ...
Gordon R. Osinski+2 more
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Impact cratering is an important and unique geologic process. The high speeds, forces and temperatures involved are quite unlike conventional endogenic processes, and the environmental consequences can be catastrophic. Kilometre-scale craters are excavated and collapse in minutes, in some cases distributing debris around the globe and exhuming deeply ...
Gordon R. Osinski+2 more
openaire +2 more sources
Icarus, 2010
Five certain impact craters and 44 additional nearly certain and probable ones have been identified on the 22% of Titan’s surface imaged by Cassini’s high-resolution radar through December 2007. The certain craters have morphologies similar to impact craters on rocky planets, as well as two with radar bright, jagged rims. The less certain craters often
Ralph D. Lorenz+5 more
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Five certain impact craters and 44 additional nearly certain and probable ones have been identified on the 22% of Titan’s surface imaged by Cassini’s high-resolution radar through December 2007. The certain craters have morphologies similar to impact craters on rocky planets, as well as two with radar bright, jagged rims. The less certain craters often
Ralph D. Lorenz+5 more
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Icarus, 2017
Abstract The majority of impact craters have circular outlines and axially symmetric morphologies. Deviation from crater circularity is caused by either target heterogeneity, a very oblique impact incidence, post-impact deformation, or by topography.
Aschauer, Johannes, Kenkmann, Thomas
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Abstract The majority of impact craters have circular outlines and axially symmetric morphologies. Deviation from crater circularity is caused by either target heterogeneity, a very oblique impact incidence, post-impact deformation, or by topography.
Aschauer, Johannes, Kenkmann, Thomas
openaire +3 more sources