Sulphate anion effect on kinetic and catalytic polarographic currents of nickel(II) aquo ion and nickel(II) complexes. Determination of the instability constant of nickel-sulphate complex

1970 ◽  
Vol 28 (2) ◽  
pp. 381-390 ◽  
Author(s):  
Ya.I. Tur'yan ◽  
O.E. Ruvinskii
1967 ◽  
Vol 114 (2) ◽  
pp. 131 ◽  
Author(s):  
William H. Metzger ◽  
Abner Brenner ◽  
Harry I. Salmon

Author(s):  
Ion Ganescu ◽  
Vasilica Muresan ◽  
Liana Simona Sbirna ◽  
Anca Ganescu ◽  
Sebastian Sbirna ◽  
...  

The paper presents a spectrophotometric study of the binary system Rh(III)-2-thioxo-4-thiazolidinone. The formation conditions and the analytical application of the formed complex for spectrophotometric determination of Rh(III) were studied. The composition of the Rh(III) chelate with this particular ligand was determined by the continuous variation method, its instability constant being Kinst = 1,61·10-8 mol2L-2.


In a series of papers the author, partly in collaboration with the late Prof. H. Kamerlingh Onnes, has recently published the results of some investigations on paramagnetism at low temperatures. Included in this work were the measurements of the principal susceptibilities of two crystals (cobalt ammonium sulphate and nickel sulphate) at temperatures ranging from about 300° K. (atmospheric temperature) down to the lowest temperature obtainable with liquid hydrogen, 14° K. These data, with the exception of those of Foëx for siderose, are the only ones yet obtained for the principal susceptibilities of paramagnetic crystals at low temperatures over any extended range of temperature. The results showed that, at not too low temperatures, the principal susceptibilities Z 1 , Z 2 , Z 3 follow the law Z n (T + Δ n = C, ( n = I, 2, 3), in which T = absolute temperature, Δ n is a constant, and C is the Curie constant which has the same value for each of the principal magnetic axes of the crystal. The constants Δ n are intimately connected with the structure of the crystal, being a function of the “spacing” of the paramagnetic atoms in the corresponding directions in the crystal. The precise connection between these quantities could not, however, be deduced, firstly, because of the present scantiness of the data, and, secondly, because the accuracy with which the Δ’s could be determined was small. The susceptibilities themselves were determined with an accuracy of about 1 per cent., but, since Δ is only an additive constant, the error in its determination is greater than that of the determination of the susceptibility. Other interesting points were raised by the results, and a continuation of the research seemed likely to give results of considerable theoretical importance and interest. The present work was undertaken in continuation of that just mentioned. It was decided to carry out the measurements over a range of temperature of from atmospheric temperature down to the lowest obtainable with the aid of liquid air, and to aim at reaching an accuracy of one part in a thousand in the measurements. For this purpose the apparatus described in the following pages was designed and constructed. I he desired accuracy was not attained in the first measurements given later in the present paper, the accuracy of these being about 1 per cent. As experience was gained with the apparatus, it was seen that the desired accuracy was probably attainable when special attention was paid to the working conditions, in particular the constancy of the temperature.


2009 ◽  
Vol 2009 ◽  
pp. 1-5 ◽  
Author(s):  
K. Ernits ◽  
K. Muska ◽  
M. Danilson ◽  
J. Raudoja ◽  
T. Varema ◽  
...  

The study on the anion effect of different Zn sources—Zn(CH3COO)2, ZnCl2, ZnI2, Zn(NO3)2and ZnSO4—on the chemical deposition of ZnS(O,OH) films revealed that the growth rate and composition of the ZnS(O,OH) layer depend on the instability constant (pK) value of the corresponding Zn-complex Zn(L)nin the chemical bath solution. In the region ofpKZn(NH3)2+>pKZn(L)nthe ZnS(O,OH) film's growth rate and ZnS concentration in films increased with the increasing pK value of the used Zn salt complex up to the pK value of theZn[NH3]2+complex and decreased in the region wherepKZn(NH3)2+<pKZn(L)n. The band gap values (around 3.6 eV in most cases) of deposited ZnS(O,OH) films did not depend on the Zn precursor's instability constant, the ZnS(O,OH) film from zinc nitrate containing bath has higher band gap energy (Eg= 3.8 eV). The maximum efficiency of CISSe and CZTSSe monograin layer solar cells was gained with ZnS(O,OH) buffer layer deposited from CBD solution containing Zn(CH3COO)2as Zn source, which provided the highest growth rate and ZnS concentration in the ZnS(O,OH) film on glass substrates.


2009 ◽  
Vol 19 (17) ◽  
pp. 4984-4987 ◽  
Author(s):  
Michelle L. Ingalsbe ◽  
Jeffrey D.St. Denis ◽  
Megan E. McGahan ◽  
Walter W. Steiner ◽  
Ronny Priefer

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.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


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