Effects of phosphorus on the stability of the passive state of Fe and Fe-Ni base glasses

1988 ◽  
Vol 39 (10) ◽  
pp. 453-462 ◽  
Author(s):  
H. Viefhaus ◽  
R. Möller ◽  
M. Janik-Czachor
Keyword(s):  
1990 ◽  
Vol 41 (11) ◽  
pp. 618-622 ◽  
Author(s):  
A. Szummer ◽  
K. Lublińska ◽  
M. Janik-Czachor
Keyword(s):  

CORROSION ◽  
1963 ◽  
Vol 19 (4) ◽  
pp. 115t-119t ◽  
Author(s):  
F. P. A. ROBINSON ◽  
F. A. FROST

Abstract The anodic polarization characteristics of gold and silver in chloride and sulfate media have been studied, employing potentiostatic techniques. It was found that gold produces an active-passive S-shaped curve, the form of which is not seriously affected by the presence of oxygen in the electrolyte. The stability of the passive state was greater in the sulfate than in the chloride media. Silver does not give a typical anodic polarization curve in NaCl solution, because formation of an AgCl film is the primary anode reaction. This film thickens and exfoliates at a current density of 2 a/sq ft. For this reason, silver could not be used as an inexpendable anode in an impressed current system containing chloride ions.


ChemInform ◽  
2010 ◽  
Vol 26 (5) ◽  
pp. no-no
Author(s):  
M. JANIK-CZACHOR ◽  
A. WOLOWIK ◽  
Z. WERNER

1990 ◽  
Vol 31 ◽  
pp. 355-360 ◽  
Author(s):  
A. Kawashima ◽  
B.-P. Zhang ◽  
H. Habazaki ◽  
K. Asami ◽  
K. Hashimoto

1999 ◽  
Vol 41 (8) ◽  
pp. 1557-1584 ◽  
Author(s):  
M. Bojinov ◽  
I. Betova ◽  
G. Fabricius ◽  
T. Laitinen ◽  
R.Raicheff d ◽  
...  

1994 ◽  
Vol 36 (11) ◽  
pp. 1921-1923 ◽  
Author(s):  
M Janik-Czachor ◽  
A Wo&Ł ◽  
Z Werner

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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