Profile Analysis Based on Repeated Measurements — A New Approach to the Analysis of Interaction

Author(s):  
Chihiro Hirotsu ◽  
Eri Ohta
2007 ◽  
Vol 46 (11) ◽  
pp. 7441-7445 ◽  
Author(s):  
M'hamed Boulakroune ◽  
Ahmed El Oualkadi ◽  
Djamel Benatia ◽  
Tahar Kezai

2002 ◽  
Vol 29 (1) ◽  
pp. 50-57 ◽  
Author(s):  
Guy Doré ◽  
Martin Flamand ◽  
Pierre Pascale

A new approach for pavement longitudinal profile analysis is described in this paper. In this approach, based on a simple moving average filtering technique, the results are expressed in terms of the proportion of the calculated international roughness index associated with different wavelengths of pavement surface deformations. The new approach has been successfully used in the assessment of the performance of Canadian Long-Term Pavement Performance (C-LTPP) test sites. The proposed analysis approach can help in identifying the source of problems causing pavement roughness. It can thus help in identifying the proper pavement rehabilitation technique. The new analysis approach has also helped in assessing the performance of the different rehabilitation techniques used in C-LTPP. It was found that 80–130 mm thick overlays give the best results in reducing roughness associated with short wavelength deformations. The benefit of these overlays is, however, limited to several years. Moreover, overlays do not have any significant impact on long wavelength deformations. It has also been found that long wavelength distortions tend to dominate the longitudinal profiles of thin pavement structures or pavements built on soft fine grained soils. Short wavelength distortions are dominant in longitudinal profiles of cracked thick pavement structures or that are built on strong soils.Key words: pavement, performance, longitudinal profile, wavelength, IRI, roughness, deformations.


1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

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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