Determination of active sulfur trioxide in sulfur trioxide-pyridine and sulfur trioxide-trimethylamine complexes

1982 ◽  
Vol 54 (7) ◽  
pp. 1216-1217 ◽  
Author(s):  
David H. Sieh ◽  
John M. Dunham
Keyword(s):  
1973 ◽  
Vol 45 (13) ◽  
pp. 2291-2292 ◽  
Author(s):  
Peggy A. Skotnicki ◽  
Alfred G. Hopkins ◽  
Chris W. Brown

2017 ◽  
Vol 726 ◽  
pp. 70-74
Author(s):  
Qian Nan Li ◽  
Man Li ◽  
Qing Dan Yuan ◽  
Dan Hua Xu

Generally, the content of sulfide and sulfate (expressed as a sulphur trioxide) in pebble and crushed stone for construction is low. So use the weight method specified in the national standard method for determination, is not only tedious and time consuming, but also not accurate enough. In this paper, with reference to the pretreatment method of the relevant national standard, rapid and accurate test results can usually be obtained for the determination of sulfur trioxide in and crushed stone for construction by using ICP-AES as a new method, greatly reducing the time of the experiment and improve the efficiency. According to the analysis of spectrum interference, 182.0 nm was selected as the best analysis of spectral line for sulfur. The detection line of this method (3S) was 0.016 mg/L, the recovery rate of the sample was between 93.3%-104.0%, and the relative standard deviation (n=6) of the parallel samples was less than 1.05%.


1950 ◽  
Vol 22 (4) ◽  
pp. 549-552 ◽  
Author(s):  
William. Seaman ◽  
J. T. Woods ◽  
H. N. Bank

2008 ◽  
pp. 67-67-5
Author(s):  
S Goswami ◽  
D Chandra
Keyword(s):  

1980 ◽  
Vol 88 (1018) ◽  
pp. 356-358
Author(s):  
Toshihisa MARUTA ◽  
Akihiko TAKEI ◽  
Giichi SUDOH

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


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