Toward the Avogadro constant-preliminary results on the molar volume of silicon

1989 ◽  
Vol 38 (2) ◽  
pp. 200-205 ◽  
Author(s):  
A. Sacconi ◽  
A.M. Peuto ◽  
W. Pasin ◽  
R. Panciera ◽  
G. Lenaers ◽  
...  
Keyword(s):  
Molar Volume ◽  
Preliminary Results ◽  
Avogadro Constant

Toward the Avogadro Constant - Preliminary Results on the Molar Volume of Silicon

1988 ◽  
Author(s):  
Sacconi ◽  
Peuto ◽  
Lenaers ◽  
Valkiers ◽  
De Bievre
Keyword(s):  
Molar Volume ◽  
Preliminary Results ◽  
Avogadro Constant

The Avogadro constant — Recent results on the molar volume of silicon

1987 ◽  
Vol IM-36 (2) ◽  
pp. 161-165 ◽  
Author(s):  
Peter Seyfried ◽  
Reiner Balhorn ◽  
Manfred Kochsiek ◽  
Andrzej F. Kozdon ◽  
H.-J. Rademacher ◽  
...  
Keyword(s):  
Molar Volume ◽  
Avogadro Constant

Determination of the Avogadro constant by accurate measurement of the molar volume of a silicon crystal

Metrologia ◽  
1999 ◽  
Vol 36 (5) ◽  
pp. 455-464 ◽  
Author(s):  
K Fujii ◽  
M Tanaka ◽  
Y Nezu ◽  
K Nakayama ◽  
H Fujimoto ◽  
...  
Keyword(s):  
Molar Volume ◽  
Silicon Crystal ◽  
Avogadro Constant

A reassessment of the molar volume of silicon and of the Avogadro constant

2001 ◽  
Vol 50 (2) ◽  
pp. 593-597 ◽  
Author(s):  
P. De Bievre ◽  
S. Valkiers ◽  
R. Kessel ◽  
P.D.P. Taylor ◽  
P. Becker ◽  
...  
Keyword(s):  
Molar Volume ◽  
Avogadro Constant

The molar volume of silicon [Avogadro constant]

1997 ◽  
Vol 46 (2) ◽  
pp. 592-595 ◽  
Author(s):  
P. De Bievre ◽  
S. Valkiers ◽  
R. Gonfiantini ◽  
P.D.P. Taylor ◽  
H. Bettin ◽  
...  
Keyword(s):  
Molar Volume ◽  
Avogadro Constant

Evaluation of the molar volume of silicon crystals for a determination of the avogadro constant

2003 ◽  
Vol 52 (2) ◽  
pp. 646-651 ◽  
Author(s):  
K. Fujii ◽  
A. Waseda ◽  
N. Kuramoto ◽  
S. Mizushima ◽  
M. Tanaka ◽  
...  
Keyword(s):  
Molar Volume ◽  
Avogadro Constant ◽  
Silicon Crystals

The O–C diagrams of minor planets − a new approach to modelling the rotation

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss
Keyword(s):  
Error Analysis ◽  
Time Dependence ◽  
Theoretical Work ◽  
Minor Planet ◽  
Minor Planets ◽  
New Approach ◽  
Preliminary Results ◽  
Ccd Observations

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.

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