Effects of elctrolytes on the stability of wetting films: Implications on seawater flotation

2018 ◽  
Vol 122 ◽  
pp. 1-9 ◽  
Author(s):  
Lei Pan ◽  
Roe-Hoan Yoon
Keyword(s):  
2003 ◽  
Vol 191 (1) ◽  
pp. 69-80 ◽  
Author(s):  
Joost H. Maas ◽  
Frans A.M. Leermakers ◽  
Gerard J. Fleer ◽  
Martinus A. Cohen Stuart

1998 ◽  
Vol 142 (2-3) ◽  
pp. 275-279 ◽  
Author(s):  
J. Mahnke ◽  
P. Müller ◽  
H.J. Schulze ◽  
K.W. Stöckelhuber ◽  
E. Weber
Keyword(s):  

1992 ◽  
Vol 152 (1) ◽  
pp. 170-182 ◽  
Author(s):  
Z.M Zorin ◽  
N.V Churaev ◽  
N.E Esipova ◽  
I.P Sergeeva ◽  
V.D Sobolev ◽  
...  

1983 ◽  
Vol 23 (02) ◽  
pp. 249-258 ◽  
Author(s):  
A.C. Hall ◽  
S.H. Collins ◽  
J.C. Melrose

Abstract The existence of thin films of water that completely wet the sand grains has long been regarded as an important feature of the Athabasca oil sands deposit. Direct microscopic evidence, however, cannot be relied on to establish whether such films are present. The existence and stability of such films, therefore, must be inferred from the relevant surface chemical forces for the oil/brine/rock system. A detailed analysis of these forces shows that the stability of these thin wetting films is critically dependent on whether the zeta potentials (and charge densities) for the two electrical double layers bounding the film are of like sign. The zeta potential and charge density for the rock/brine interface will in almost all cases be negative in sign. Therefore, a requirement for the stability of a wetting film will be that these quantities are also negative at the brine/oil interface. New measurements of the electrophoretic mobility of small particles of Athabasca bitumen suspended in an aqueous phase are reported. These data show that the zeta potential at the bitumen/water interface is strongly negative. Consequently, these results suppose the hypothesis that wetting films will be stable in this instance. Introduction The great economic potential and geological significance of the Athabasca oil sands, as well as ready accessibility of outcrop specimens, have motivated extensive investigations of their chemical and physical properties for the past several decades. Although many details remain still unresolved, there is broad agreement regarding the gross physical nature of the quartz/bitumen/water mixture that constitutes the bulk of the resource. In particular, it is usually postulated that, even in the particular, it is usually postulated that, even in the bitumen-rich deposits where water content is very low, the aqueous phase is distributed in the form of continuous films that surround the quartz grains. In other words, the grains themselves are separated from the bitumen phase by envelopes of water. These envelopes are presumed to be much thicker than a simple monolayer or bilayer of water molecules (0.3 to 0.6 nm). The first published suggestion of such an arrangement was appended as a reader's comment to a general review of Athabasca oil-sands geology. Since then, others have reaffirmed this idea, occasionally pointing out also that, while present in the Athabasca material, such aqueous envelopes, separating oil from sand, are not an essential feature of all oil and tar sands. It is of some interest, however, so far as the Athabasca oil sands are concerned, that no direct observation of water films of greater-than-molecular thickness seems ever to have been made: thus, the evidence is, to date, indirect and equivocal. There is no doubt that the question of whether such wetting films are present is of more than academic importance. Rapid, complete separation of the Athabasca bitumen from sand is a key requirement for both current methods of mining and future in-situ technology. The modeling and optimization of such processes clearly will depend on a correct interpretation of the physical mechanisms involved, and this in turn requires a valid assessment of the initial physical state of the system. SPEJ P. 249


1982 ◽  
Vol 99 ◽  
pp. 605-613
Author(s):  
P. S. Conti

Conti: One of the main conclusions of the Wolf-Rayet symposium in Buenos Aires was that Wolf-Rayet stars are evolutionary products of massive objects. Some questions:–Do hot helium-rich stars, that are not Wolf-Rayet stars, exist?–What about the stability of helium rich stars of large mass? We know a helium rich star of ∼40 MO. Has the stability something to do with the wind?–Ring nebulae and bubbles : this seems to be a much more common phenomenon than we thought of some years age.–What is the origin of the subtypes? This is important to find a possible matching of scenarios to subtypes.


1999 ◽  
Vol 173 ◽  
pp. 309-314 ◽  
Author(s):  
T. Fukushima

AbstractBy using the stability condition and general formulas developed by Fukushima (1998 = Paper I) we discovered that, just as in the case of the explicit symmetric multistep methods (Quinlan and Tremaine, 1990), when integrating orbital motions of celestial bodies, the implicit symmetric multistep methods used in the predictor-corrector manner lead to integration errors in position which grow linearly with the integration time if the stepsizes adopted are sufficiently small and if the number of corrections is sufficiently large, say two or three. We confirmed also that the symmetric methods (explicit or implicit) would produce the stepsize-dependent instabilities/resonances, which was discovered by A. Toomre in 1991 and confirmed by G.D. Quinlan for some high order explicit methods. Although the implicit methods require twice or more computational time for the same stepsize than the explicit symmetric ones do, they seem to be preferable since they reduce these undesirable features significantly.


Author(s):  
Godfrey C. Hoskins ◽  
V. Williams ◽  
V. Allison

The method demonstrated is an adaptation of a proven procedure for accurately determining the magnification of light photomicrographs. Because of the stability of modern electrical lenses, the method is shown to be directly applicable for providing precise reproducibility of magnification in various models of electron microscopes.A readily recognizable area of a carbon replica of a crossed-line diffraction grating is used as a standard. The same area of the standard was photographed in Phillips EM 200, Hitachi HU-11B2, and RCA EMU 3F electron microscopes at taps representative of the range of magnification of each. Negatives from one microscope were selected as guides and printed at convenient magnifications; then negatives from each of the other microscopes were projected to register with these prints. By deferring measurement to the print rather than comparing negatives, correspondence of magnification of the specimen in the three microscopes could be brought to within 2%.


Author(s):  
E. R. Kimmel ◽  
H. L. Anthony ◽  
W. Scheithauer

The strengthening effect at high temperature produced by a dispersed oxide phase in a metal matrix is seemingly dependent on at least two major contributors: oxide particle size and spatial distribution, and stability of the worked microstructure. These two are strongly interrelated. The stability of the microstructure is produced by polygonization of the worked structure forming low angle cell boundaries which become anchored by the dispersed oxide particles. The effect of the particles on strength is therefore twofold, in that they stabilize the worked microstructure and also hinder dislocation motion during loading.


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