impact shock
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ACS Nano ◽  
2021 ◽  
Vol 15 (2) ◽  
pp. 2439-2446
Author(s):  
Jinho Hyon ◽  
Manny Gonzales ◽  
Jason K. Streit ◽  
Omri Fried ◽  
Olawale Lawal ◽  
...  


2020 ◽  
Vol 80 ◽  
pp. 105131 ◽  
Author(s):  
Roberto Sanchis-Sanchis ◽  
Cristina Blasco-Lafarga ◽  
Andrés Camacho-García ◽  
Alberto Encarnación-Martínez ◽  
Pedro Pérez-Soriano


2020 ◽  
Vol 192 ◽  
pp. 105041
Author(s):  
R S Thombre ◽  
F. Gomez ◽  
R. Parkhe ◽  
K. Kaur ◽  
P. Vaishampayan ◽  
...  
Keyword(s):  


2020 ◽  
Vol 117 (41) ◽  
pp. 25310-25318 ◽  
Author(s):  
Fabrizio Nestola ◽  
Cyrena A. Goodrich ◽  
Marta Morana ◽  
Anna Barbaro ◽  
Ryan S. Jakubek ◽  
...  

The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studies have proposed their formation at static pressures >20 GPa in a large planetary body, like diamonds formed deep within Earth’s mantle. We investigated fragments of three diamond-bearing ureilites (two from the Almahata Sitta polymict ureilite and one from the NWA 7983 main group ureilite). In NWA 7983 we found an intimate association of large monocrystalline diamonds (up to at least 100 µm), nanodiamonds, nanographite, and nanometric grains of metallic iron, cohenite, troilite, and likely schreibersite. The diamonds show a striking texture pseudomorphing inferred original graphite laths. The silicates in NWA 7983 record a high degree of shock metamorphism. The coexistence of large monocrystalline diamonds and nanodiamonds in a highly shocked ureilite can be explained by catalyzed transformation from graphite during an impact shock event characterized by peak pressures possibly as low as 15 GPa for relatively long duration (on the order of 4 to 5 s). The formation of “large” (as opposed to nano) diamond crystals could have been enhanced by the catalytic effect of metallic Fe-Ni-C liquid coexisting with graphite during this shock event. We found no evidence that formation of micrometer(s)-sized diamonds or associated Fe-S-P phases in ureilites require high static pressures and long growth times, which makes it unlikely that any of the diamonds in ureilites formed in bodies as large as Mars or Mercury.





2019 ◽  
pp. 325-338
Author(s):  
Mohsen Shafizadeh ◽  
Nicola Theis ◽  
Keith Davids

The aim of this study was to examine strategies to absorb impact shock during RaceRunning in participants with neurological motor disorders. For this purpose, 8 RaceRunning athletes (4 male and 4 female) voluntarily took part in the study. Each participant performed a series of 100-m sprints with a RaceRunning bike. Acceleration of the tibia and head was measured with 2 inertial measurement units and used to calculate foot-impact shock measures. Results showed that RaceRunning pattern was characterized by a lack of impact peak in foot–ground contact time and the existence of an active peak after foot contact. Due to the ergonomic properties of the RaceRunning bike, shock is attenuated throughout the stance phase. In conclusion, the results revealed that RaceRunning athletes with neurological motor disorders are capable of absorbing impact shock during assisted RaceRunning using a strategy that mimics runners without disabilities.



2018 ◽  
Vol 124 (20) ◽  
pp. 205105 ◽  
Author(s):  
David J. Walters ◽  
Ayan Biswas ◽  
Earl C. Lawrence ◽  
Devin C. Francom ◽  
Darby J. Luscher ◽  
...  


2018 ◽  
Vol 35 (1) ◽  
pp. 77-88 ◽  
Author(s):  
M. Eskandari ◽  
M. A. Mohtadi-Bonab ◽  
M. Yeganeh ◽  
J. A. Szpunar ◽  
A. G. Odeshi


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