Results 241 to 250 of about 35,040 (307)
Seismic resurfacing of 433 Eros indicative of a highly dissipative interior for large near-Earth asteroids. [PDF]
Ballouz RL +6 more
europepmc +1 more source
Double-Pulse Femtosecond Laser Fabrication of Highly Ordered Periodic Structures on Au Thin Films Enabling Low-Cost Plasmonic Applications. [PDF]
Fraggelakis F +9 more
europepmc +1 more source
Experimental investigation and parametric optimization of machinability and surface characteristics in wire EDM of Inconel 718. [PDF]
Kar S +5 more
europepmc +1 more source
Monlunabant in adults with obesity and metabolic syndrome: Open‐label extension of a phase 2a trial
Diabetes, Obesity and Metabolism, Volume 28, Issue 5, Page 4366-4371, May 2026.
Filip K. Knop +10 more
wiley +1 more source
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Annual Review of Earth and Planetary Sciences, 1999
▪ 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 ...
H. J. Melosh, B. A. Ivanov
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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 ...
H. J. Melosh, B. A. Ivanov
openaire +1 more source
Meteorite impact crater inventory of turkey
Proceedings of 2nd International Conference on Recent Advances in Space Technologies, 2005. RAST 2005., 2006Interplanetary space is populated with large numbers of small bodies known as meteorites, which are in orbits that can intersect those of planets and moons. Therefore, individual impacts appear on the surfaces of planetary bodies which are called impact craters.
Sengul, E +4 more
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Laboratory Craters: Modeling Experiments for Meteorite Impact Craters?
IEEE Transactions on Plasma Science, 2008In this paper, we reveal the feasibility of obtaining laboratory craters to investigate planetary events such as meteorite craters. Experiments were performed by using 0.44-mum laser beam with energy of les15 J in 350 ps (full-width at half-maximum) on aluminum targets.
Tara Desai +5 more
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Advances in Space Research, 1991
Abstract A summary of experimental and theoretical studies of atmosphere-related phenomena accompanying high velocity impact processes is presented, including asteroid and comet passage through the atmosphere, their impact on the surfaces of different planetary bodies, blast waves in the atmosphere and their influence on surface life. These phenomena
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Abstract A summary of experimental and theoretical studies of atmosphere-related phenomena accompanying high velocity impact processes is presented, including asteroid and comet passage through the atmosphere, their impact on the surfaces of different planetary bodies, blast waves in the atmosphere and their influence on surface life. These phenomena
openaire +1 more source

