scholarly journals Micromachined nanocrystalline graphite membranes for gas separation

Carbon ◽  
2018 ◽  
Vol 138 ◽  
pp. 125-133 ◽  
Author(s):  
S.J. Fishlock ◽  
S.H. Pu ◽  
G. Bhattacharya ◽  
Yisong Han ◽  
J. McLaughlin ◽  
...  
Author(s):  
C.E. Voegele-Kliewer ◽  
A.D. McMaster ◽  
G.W. Dirks

Materials other than polymers, e.g. ceramic silicates, are currently being investigated for gas separation processes. The permeation characteristics of one such material, Vycor (Corning Glass #1370), have been reported for the separation of hydrogen from hydrogen iodide. This paper will describe the electron microscopy techniques applied to reveal the porous microstructure of a Vycor membrane. The application of these techniques has led to an increased understanding in the relationship between the substructure and the gas transport properties of this material.


2019 ◽  
Author(s):  
Anders Andreasen

In this article the optimization of a realistic oil and gas separation plant has been studied. Two different fluids are investigated and compared in terms of the optimization potential. Using Design of Computer Experiment (DACE) via Latin Hypercube Sampling (LHS) and rigorous process simulations, surrogate models using Kriging have been established for selected model responses. The surrogate models are used in combination with a variety of different evolutionary algorithms for optimizing the operating profit, mainly by maximizing the recoverable oil production. A total of 10 variables representing pressure and temperature various key places in the separation plant are optimized to maximize the operational profit. The optimization is bounded in the variables and a constraint function is included to ensure that the optimal solution allows export of oil with an RVP < 12 psia. The main finding is that, while a high pressure is preferred in the first separation stage, apparently a single optimal setting for the pressure in downstream separators does not appear to exist. In the second stage separator apparently two different, yet equally optimal, settings are revealed. In the third and final separation stage a correlation between the separator pressure and the applied inlet temperature exists, where different combinations of pressure and temperature yields equally optimal results.<br>


2010 ◽  
Vol 25 (5) ◽  
pp. 449-456 ◽  
Author(s):  
Lin LI ◽  
Tong-Hua WANG ◽  
Yi-Ming CAO ◽  
Jie-Shan QIU

2009 ◽  
Vol 25 (1) ◽  
pp. 47-52
Author(s):  
Xuan-Ying ZHAO ◽  
Tong-Hua WANG ◽  
Lin LI ◽  
Ying LIU ◽  
Yi-Ming CAO
Keyword(s):  

2010 ◽  
Vol 3 (1) ◽  
pp. 1-16 ◽  
Author(s):  
Kailash Ch. Khulbe ◽  
Chaoyang Y. Feng ◽  
Takeshi Matsuura

Carbon ◽  
2020 ◽  
Author(s):  
Yunjiao Wang ◽  
Min Cheng ◽  
Liang Wang ◽  
Daming Zhou ◽  
Shixuan He ◽  
...  

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Q. H. S. Chan ◽  
A. Stephant ◽  
I. A. Franchi ◽  
X. Zhao ◽  
R. Brunetto ◽  
...  

AbstractUnderstanding the true nature of extra-terrestrial water and organic matter that were present at the birth of our solar system, and their subsequent evolution, necessitates the study of pristine astromaterials. In this study, we have studied both the water and organic contents from a dust particle recovered from the surface of near-Earth asteroid 25143 Itokawa by the Hayabusa mission, which was the first mission that brought pristine asteroidal materials to Earth’s astromaterial collection. The organic matter is presented as both nanocrystalline graphite and disordered polyaromatic carbon with high D/H and 15N/14N ratios (δD =  + 4868 ± 2288‰; δ15N =  + 344 ± 20‰) signifying an explicit extra-terrestrial origin. The contrasting organic feature (graphitic and disordered) substantiates the rubble-pile asteroid model of Itokawa, and offers support for material mixing in the asteroid belt that occurred in scales from small dust infall to catastrophic impacts of large asteroidal parent bodies. Our analysis of Itokawa water indicates that the asteroid has incorporated D-poor water ice at the abundance on par with inner solar system bodies. The asteroid was metamorphosed and dehydrated on the formerly large asteroid, and was subsequently evolved via late-stage hydration, modified by D-enriched exogenous organics and water derived from a carbonaceous parent body.


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