Purification of zinc ammoniacal leaching solution by cementation: Determination of optimum process conditions with experimental design by Taguchi's method

2006 ◽  
Vol 51 (2) ◽  
pp. 157-164 ◽  
Author(s):  
J MOGHADDAM ◽  
R SARRAFMAMOORY ◽  
M ABDOLLAHY ◽  
Y YAMINI
2014 ◽  
Vol 1004-1005 ◽  
pp. 1186-1192
Author(s):  
Yan Song Li ◽  
Da Wei Wang

The development of standard simple of tin bronze for casting is presented,design of composition, selection melting temperature 1150 °C, put into 0.2m3/kg argon gas, stirring with 100rpm for 1min, keeping temperature for 30min as the optimum process conditions, coarse and fine tests of homogeneity with data analyses, determination of standard values and standard deviation. The homogeneity and standard values of samples meet the national standard GB/T15000 and YS/T409-1998. The standard sample series has ratification as National Reference Materials (GSB 04-2707-2011) by National Technical Commission on Reference Materials.


2008 ◽  
Vol 90 (2-4) ◽  
pp. 115-120 ◽  
Author(s):  
M. Taghizadeh ◽  
R. Ghasemzadeh ◽  
S.N Ashrafizadeh ◽  
K. Saberyan ◽  
M. Ghanadi Maragheh

1978 ◽  
Vol 48 ◽  
pp. 7-29
Author(s):  
T. E. Lutz

This review paper deals with the use of statistical methods to evaluate systematic and random errors associated with trigonometric parallaxes. First, systematic errors which arise when using trigonometric parallaxes to calibrate luminosity systems are discussed. Next, determination of the external errors of parallax measurement are reviewed. Observatory corrections are discussed. Schilt’s point, that as the causes of these systematic differences between observatories are not known the computed corrections can not be applied appropriately, is emphasized. However, modern parallax work is sufficiently accurate that it is necessary to determine observatory corrections if full use is to be made of the potential precision of the data. To this end, it is suggested that a prior experimental design is required. Past experience has shown that accidental overlap of observing programs will not suffice to determine observatory corrections which are meaningful.


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