Upgrading of palmitic acid to diesel-like fuels over Ni@HZSM-5 bi-functional catalysts through the in situ encapsulation method

2021 ◽  
Vol 511 ◽  
pp. 111715
Author(s):  
Chen Gao ◽  
Jimei Zhang ◽  
Enhui Xing ◽  
Yongbing Xie ◽  
He Zhao ◽  
...  
1959 ◽  
Vol 196 (6) ◽  
pp. 1238-1241 ◽  
Author(s):  
Y. Stein ◽  
B. Shapiro

Up to 60% of i.v. injected doses of 1-C14 palmitic acid was found in the liver 15 minutes after injection, two thirds in the form of triglycerides and the rest as phospholipids. Almost no radioactive UFA could be demonstrated in the liver or in blood plasma. Thereafter, the activity in the triglyceride fraction fell rapidly, only 50% remaining after 1 hour. At the same time the phospholipid activity increased. With 1-C14 linoleic acid a similar pattern was found, except that the percentage retained in the liver was lower and maximum retention was found after 5 minutes. Fifteen minutes after injection of 1-C14 palmitate most of the radioactive glycerides in the liver were found in the microsomes and mitochondria, with very little in the floating fat. Equilibration between these cytoplasmatic particles occurred only after 2 hours. Perfusion of the liver in situ with blood or blood substitutes, after various periods following 1-C14 palmitic acid injection, caused a release of about 5–20% of the liver triglycerides and 0.5–2% of the liver phospholipids per hour.


Atmosphere ◽  
2018 ◽  
Vol 9 (12) ◽  
pp. 471 ◽  
Author(s):  
Ben Woden ◽  
Maximilian Skoda ◽  
Matthew Hagreen ◽  
Christian Pfrang

This paper describes experiments on the ageing of a monolayer model for the air–water interface of marine aerosols composed of a typical glycolipid, galactocerebroside (GCB). Lipopolysaccharides have been observed in marine aerosols, and GCB is used as a proxy for these more complex lipopolysaccharides. GCB monolayers are investigated as pure films, as mixed films with palmitic acid, which is abundant in marine aerosols and forms a stable attractively mixed film with GCB, particularly with divalent salts present in the subphase, and as mixed films with palmitoleic acid, an unsaturated analogue of palmitic acid. Such mixed films are more realistic models of atmospheric aerosols than simpler single-component systems. Neutron reflectometry (NR) has been combined in situ with Fourier transform infra-red reflection absorption spectroscopy (IRRAS) in a pioneering analysis and reaction setup designed by us specifically to study mixed organic monolayers at the air–water interface. The two techniques in combination allow for more sophisticated observation of multi-component monolayers than has previously been possible. The structure at the air–water interface was also investigated by complementary Brewster angle microscopy (BAM). This study looks specifically at the oxidation of the organic films by nitrate radicals (NO3•), the key atmospheric oxidant present at night. We conclude that NO3• oxidation cannot fully remove a cerebroside monolayer from the surface on atmospherically relevant timescales, leaving its saturated tail at the interface. This is true for pure and salt water subphases, as well as for single- and two-component films. The behaviour of the unsaturated tail section of the molecule is more variable and is affected by interactions with co-deposited species. Most surprisingly, we found that the presence of CaCl2 in the subphase extends the lifetime of the unsaturated tail substantially—a new explanation for longer residence times of materials in the atmosphere compared to lifetimes based on laboratory studies of simplified model systems. It is thus likely that aerosols produced from the sea-surface microlayer at night will remain covered in surfactant molecules on atmospherically relevant timescales with impact on the droplet’s surface tension and on the transport of chemical species across the air–water interface.


1984 ◽  
Vol 75 ◽  
pp. 743-759 ◽  
Author(s):  
Kerry T. Nock

ABSTRACTA mission to rendezvous with the rings of Saturn is studied with regard to science rationale and instrumentation and engineering feasibility and design. Future detailedin situexploration of the rings of Saturn will require spacecraft systems with enormous propulsive capability. NASA is currently studying the critical technologies for just such a system, called Nuclear Electric Propulsion (NEP). Electric propulsion is the only technology which can effectively provide the required total impulse for this demanding mission. Furthermore, the power source must be nuclear because the solar energy reaching Saturn is only 1% of that at the Earth. An important aspect of this mission is the ability of the low thrust propulsion system to continuously boost the spacecraft above the ring plane as it spirals in toward Saturn, thus enabling scientific measurements of ring particles from only a few kilometers.


Author(s):  
R. E. Herfert

Studies of the nature of a surface, either metallic or nonmetallic, in the past, have been limited to the instrumentation available for these measurements. In the past, optical microscopy, replica transmission electron microscopy, electron or X-ray diffraction and optical or X-ray spectroscopy have provided the means of surface characterization. Actually, some of these techniques are not purely surface; the depth of penetration may be a few thousands of an inch. Within the last five years, instrumentation has been made available which now makes it practical for use to study the outer few 100A of layers and characterize it completely from a chemical, physical, and crystallographic standpoint. The scanning electron microscope (SEM) provides a means of viewing the surface of a material in situ to magnifications as high as 250,000X.


Sign in / Sign up

Export Citation Format

Share Document