Present State of the Determination of Thermodynamic Temperatures near the Freezing Point of Silver by Absolute Cryoradiometry

Metrologia ◽  
1991 ◽  
Vol 28 (3) ◽  
pp. 243-246 ◽  
Author(s):  
J Fischer ◽  
Fu Lei ◽  
M Stock

The equilibrium diagram of the system silver-zinc has been investigated by thermal, microscopic, and X-ray methods. This has enabled the following points to be established: (1) The depression of the freezing-point of silver by zinc is slightly greater than that produced by equal atomic percentages of indium. This does not confirm the hypothesis of whole-number liquidus factors previously suggested by Hume-Rothery, Mabbott and Channell-Evans (1934). (2) The solidus and liquidus curves for the β -phase do not coincide at 50 atomic % of zinc as was proposed by B. G. Petrenko (1929). The freezing range of the equiatomic alloy is approximately 3 1/2 °. (3) The determination of phase boundaries by X-ray methods with quenched filings is unreliable for this class of alloy, and its limitations are discussed.


1966 ◽  
Vol 49 (3) ◽  
pp. 511-515 ◽  
Author(s):  
R W Henningson

Abstract Bath level, sample temperature, rate of stirring, degree of supercooling, sample size, sample isolation, and refreezing of the sample were the variables in the thermistor cryoscopic method for the determination of the freezing point value of milk chosen for study. Freezing point values were determined for two samples of milk and two secondary salt standards utilizing eight combinations of the seven variables in two test patterns. The freezing point value of the salt standards ranged from –0.413 to –0.433°C and from –0.431 to –0.642°C. The freezing point values of the milk samples ranged from –0.502 to –0.544°C and from –0.518 to –0.550°C. Statistical analysis of the data showed that sample isolation was a poor procedure and that other variables produced changes in the freezing point value ranging from 0.001 to 0.011°C. It is recommended that specific directions be instituted for the thermistor cryoscopic method, 15.040–15.041, and that the method be subjected to a collaborative study.


2014 ◽  
Vol 18 (12) ◽  
pp. 3339-3344 ◽  
Author(s):  
Graeme A. Snook ◽  
Katherine McGregor ◽  
Andrew J. Urban

1869 ◽  
Vol 6 ◽  
pp. 517-518
Author(s):  
W. Pitrie

This paper is a compilation and discussion of all the best determinations of the sun's mean distance and parallax within the last few years, and up to the present time. The comparative weights to be given to the different observations or results are entered into at length, on principles which are stated, and a final mean of the whole is arrived at, giving for the solar parallax 8·″877. This is then compared with the result of the so-called Great Pyramid Sun Distance, which, combined with the best modern determination of the size and shape of the earth, gives a parallax of 8·″876.


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