scholarly journals The determination of convex bodies from the size and shape of their projections and sections

2009 ◽  
Author(s):  
Paul Goodey
Keyword(s):  
1983 ◽  
Vol 48 (1) ◽  
pp. 192-198 ◽  
Author(s):  
Tomáš Boublík

The excess entropy of mixing of mixtures of hard spheres and spherocylinders is determined from an equation of state of hard convex bodies. The obtained dependence of excess entropy on composition was used to find the accuracy of determining ΔSE from relations employed for the correlation and prediction of vapour-liquid equilibrium. Simple rules were proposed for establishing the mean parameter of nonsphericity for mixtures of hard bodies of different shapes allowing to describe the P-V-T behaviour of solutions in terms of the equation of state fo pure substance. The determination of ΔSE by means of these rules is discussed.


Mathematika ◽  
1993 ◽  
Vol 40 (2) ◽  
pp. 161-168 ◽  
Author(s):  
R. J. Gardner ◽  
A. Volčič
Keyword(s):  

2020 ◽  
Author(s):  
Haohang Huang ◽  
◽  
Jiayi Luo ◽  
Erol Tutumluer ◽  
John Hart ◽  
...  

2005 ◽  
Vol 20 ◽  
pp. 67-81 ◽  
Author(s):  
Sara Brunetti ◽  
Alain Daurat
Keyword(s):  

2001 ◽  
Vol 12 (1) ◽  
pp. 87-94 ◽  
Author(s):  
Clara E. Huisinga-Fischer ◽  
Frans W. Zonneveld ◽  
J. Michiel Vaandrager ◽  
Birte Prahl-Andersen ◽  
Barry L. Eppley

2008 ◽  
Vol 94 (7) ◽  
pp. 2706-2715 ◽  
Author(s):  
Achilleas Tsortos ◽  
George Papadakis ◽  
Konstantinos Mitsakakis ◽  
Kathryn A. Melzak ◽  
Electra Gizeli

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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