Ultradispersed diamond powders of detonation nature for polishing X-ray mirrors

Author(s):  
N.I. Chkhalov ◽  
M.V. Fedorchenko ◽  
E.P. Kruglyakov ◽  
A.I. Volokhov ◽  
K.S. Baraboshkin ◽  
...  
1996 ◽  
Vol 423 ◽  
Author(s):  
Dong-Gu Lee ◽  
Rajiv K. Singh

AbstractWe have developed a method for <111> oriented diamond film synthesis using micron-sized diamond particles. Different size of diamond powders were electrophoretically seeded on silicon substrates using diamond suspensions in organic solvents (acetone, methanol, and ethanol). Diamond suspension in acetone was found to be the best for obtaining uniform diamond seeding by electrophoresis. The thickness of diamond seeded films was changed by varying the applied voltage to observe the effect on the orientation of diamond particles. Then diamond films were deposited by the hot filament chemical vapor deposition (HFCVD) process. A preferred orientation with <111> direction normal to the substrate was obtained for monolayer coatings. The surface morphology, crystal orientation, and quality of diamond films were investigated using scanning electron microscopy, x-ray diffractometry, and Raman spectroscopy.


1997 ◽  
Vol 499 ◽  
Author(s):  
A. Witek ◽  
B. Palosz ◽  
S. Stel'Makh ◽  
S. Gierlotka ◽  
R. Pielaszek ◽  
...  

ABSTRACTCompacts of polycrystalline diamond were made in toroid-type high-pressure camera under the pressure of 8 GPa using temperatures between 800 to 2150°C without the use of additive components. Nanocrystalline commercial DALAN, and microcrystalline ASM diamond powders were used. The compacts were characterized by helium pycnometry, Vickers hardness measurements, X-ray diffraction and SEM methods.The starting and sintered nanocrystalline grain compacts were found to have strongly one-dimensionally disordered cubic modification. The nanocrystalline powder had a bimodal grain size distribution function as determined from X-ray diffraction data and ab initio intensity calculations performed with the use of Debye functions. It was found that neither the grain size nor one-dimensional disordering change under high-pressure high-temperature conditions. There is a general tendency in a decrease of density of compacts with increase in the sintering temperature what resulting partly from graphitization above 1000–1200°C. The main factor which determines the density of the diamond compacts is closed porosity. Typically, the nanocrystalline diamond compacts sintered from 30 sec. to 6 min. have densities around 90% of the theoretical value. Their Vickers microhardness is 24 GPa and less.


2014 ◽  
Vol 56 (11) ◽  
pp. 2343-2347 ◽  
Author(s):  
M. D. Sharkov ◽  
M. E. Boiko ◽  
S. N. Ivashevskaya ◽  
S. G. Konnikov

1979 ◽  
Vol 18 (8) ◽  
pp. 575-577 ◽  
Author(s):  
V. G. Chuprina ◽  
G. P. Volk ◽  
I. A. Lavrinenko ◽  
Yu. V. Naidich

2009 ◽  
Vol 255 (7) ◽  
pp. 4322-4328 ◽  
Author(s):  
Momtchil Dimitrov ◽  
Ljubomira Ivanova ◽  
Daniela Paneva ◽  
Tanya Tsoncheva ◽  
Stavry Stavrev ◽  
...  

Carbon ◽  
1991 ◽  
Vol 29 (4-5) ◽  
pp. 665-668 ◽  
Author(s):  
V.L Kuznetsov ◽  
M.N Aleksandrov ◽  
I.V Zagoruiko ◽  
A.L Chuvilin ◽  
E.M Moroz ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


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