2003
DOI: 10.1016/s0168-583x(03)00876-0
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Crater formation and sputtering by cluster impacts

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Cited by 14 publications
(4 citation statements)
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“…Craters are part of the widespread phenomena observed in nature, going from impact meteorite craters to volcanic structures. Studies of crater morphologies have a wide range of applications, going from puzzling crater formation in drying paint [1] to molecular dynamics [2,3,4]. Among the main applications to natural phenomena, aside from meteorite impact crater, are the formation and growth of volcanic edifices, by successive ejecta emplacement and/or erosion.…”
Section: Introductionmentioning
confidence: 99%
“…Craters are part of the widespread phenomena observed in nature, going from impact meteorite craters to volcanic structures. Studies of crater morphologies have a wide range of applications, going from puzzling crater formation in drying paint [1] to molecular dynamics [2,3,4]. Among the main applications to natural phenomena, aside from meteorite impact crater, are the formation and growth of volcanic edifices, by successive ejecta emplacement and/or erosion.…”
Section: Introductionmentioning
confidence: 99%
“…Almost all of the Ar atoms in the incident cluster leave the target and the crater-like damage is left on the surface. This characteristic crater formation has been confirmed by MD simulations of other materials [21][22][23] and by experiments [24,25]. During the crater formation process, some atoms at the rim may gain enough energy to leave the target, which is a feature of sputtering with huge clusters [26][27][28].…”
Section: Large Gas Cluster Impact and Crater Formationmentioning
confidence: 54%
“…As discussed, this is the scale of roughness that is expected to contribute to field emission, direct evidence that GCIB is effective at smoothing features that could not be smoothed even using the best of previous mechanical polishing techniques for non-planar electrodes. The effective size scale for GCIB polishing is determined by the properties of the surface, the average size of craters made by individual cluster impacts (typically in the range of 10-20 nm for high energy Ar clusters [9][10][11][12][13]), and by the applied GCIB dose. We have seen similar results when treating Ti surfaces with similar initial polish using Ar GCIB.…”
Section: Stainless Steel Electrode Materialsmentioning
confidence: 99%