The principle of strictly increasing mixing character in incompatible general measurement

1982 ◽  
Vol 15 (6) ◽  
pp. 1775-1783 ◽  
Author(s):  
F Herbut ◽  
I D Ivanovic
2021 ◽  
Vol 11 (3) ◽  
pp. 1287
Author(s):  
Tianyan Chen ◽  
Jinsong Lin ◽  
Deyu Wu ◽  
Haibin Wu

Based on the current situation of high precision and comparatively low APA (absolute positioning accuracy) in industrial robots, a calibration method to enhance the APA of industrial robots is proposed. In view of the "hidden" characteristics of the RBCS (robot base coordinate system) and the FCS (flange coordinate system) in the measurement process, a comparatively general measurement and calibration method of the RBCS and the FCS is proposed, and the source of the robot terminal position error is classified into three aspects: positioning error of industrial RBCS, kinematics parameter error of manipulator, and positioning error of industrial robot end FCS. The robot position error model is established, and the relation equation of the robot end position error and the industrial robot model parameter error is deduced. By solving the equation, the parameter error identification and the supplementary results are obtained, and the method of compensating the error by using the robot joint angle is realized. The Leica laser tracker is used to verify the calibration method on ABB IRB120 industrial robot. The experimental results show that the calibration method can effectively enhance the APA of the robot.


Solar Physics ◽  
2019 ◽  
Vol 294 (10) ◽  
Author(s):  
James Pickering ◽  
Huw Morgan

Abstract The increasing size of solar datasets demands highly efficient and robust analysis methods. This paper presents an approach that can increase the computational efficiency of differential emission measure (DEM) inversions by an order of magnitude or higher, with the efficiency factor increasing with the size of the input dataset. The method, named the Gridded Solar Iterative Temperature Emission Solver (Grid-SITES) is based on grouping pixels according to the similarity of their intensities in multiple channels, and solving for one DEM per group. This is shown to be a valid approach, given a sufficiently high number of grid bins for each channel. The increase in uncertainty arising from the quantisation of the input data is small compared to the general measurement and calibration uncertainties. In this paper, we use the Solar Iterative Temperature Emission Solver (SITES) as the core method for the DEM inversion, although Grid-SITES provides a general framework which may be used with any DEM inversion method, or indeed any large multi-dimensional data inversion problem. The method is particularly efficient for processing larger images, offering a factor of 30 increase in speed for a 10 megapixel image. For a time series of observations, the gridded results can be passed sequentially to each new image, with new populated bins added as required. This process leads to increasing efficiency with each new image, with potential for a ${\approx\,}100$≈100 increase in efficiency dependent on the size of the images.


2020 ◽  
Vol 34 (14n16) ◽  
pp. 2040097
Author(s):  
Zhuang Su

The mixing within a full depth lock-exchange gravity current was investigated experimentally with planar laser-induced fluorescence PLIF. The scalar edge of the gravity current was identified via an edge detection algorithm. A strong mixing region located along this edge was extracted from the flow field and analyzed. A dimensionless background potential energy was defined to characterize the local mixing rate in this region, which showed a two-stage behavior. In the section near the nose, mixing rate oscillates strongly under the influence of the lobe and cleft shifting, while in the upper part, the mixing rate grows gradually under the mechanism of billows rolling up.


2018 ◽  
Vol 22 (3) ◽  
pp. 278-289 ◽  
Author(s):  
Marion S. Aftanas ◽  
Joanna Solomon

A review of the historical measurement theory literature in psychology reveals a recurring focus on a physical rather than a psychological model of the measurement process, whereas the active measurement research literature points to an emphasis on elements of a psychological measurement process. On the basis of the relevant portions of these anomalous findings the authors outline parts of a general measurement structure for psychology that begins with an essential theoretical base. The review first explores a century-old statement that developed a promising starting point within test development. This is followed by a diversionary statement based on physical measurement that mandated discussions of measurement in psychology to a physical model. The statement appeared to be countered by the theory of scale types ( Stevens, 1946 ), which provided a promising element of the psychological measurement process. The legacy of the theory of scales, however, resulted in confusion and inconsistency about the specifics of psychological measurement. After reviewing some of the contributions in the research literature, a conciliation of the positive theory efforts of the past and the protocols for a measurement process are presented that is based upon the standard system of measurement ( Aftanas, 1988 , 2006 ) as the basic theoretically necessary element of measurement. The theoretical framework based on the standard system promises not only to integrate the components of measurement, and categories of psychological measurement that have been referenced in the past, but also to provide an easily assimilated protocol that can serve as a basis for future research and pedagogical exposition.


2020 ◽  
Vol 495 (1) ◽  
pp. 621-636 ◽  
Author(s):  
C Jiang ◽  
M Cunha ◽  
J Christensen-Dalsgaard ◽  
QS Zhang

ABSTRACT Because of the high-quality data of space missions, the detection of mixed modes has become possible in numerous stars. In this work, we investigate how the mixing character of dipolar mixed modes changes with stellar evolution, as well as with frequency within each stellar model. This is achieved by monitoring the variations in the coupling strength and the period spacing of dipolar mixed modes in red-giant models. These parameters are measured by fitting the asymptotic expansion of mixed modes to the model frequencies of a grid of red-giant models with masses between 1.0 and 2.0 M⊙ and three different chemical abundances. The coupling strength and the period spacing decrease with stellar evolution. We find that the slopes of their decreasing trends depend on the radial order of the pressure mode component. A non-negligible increase of the coupling strength with frequency by up to around 40 per cent is found in the observable frequency range for a set of red-giant models. On the contrary, no significant changes of the period spacing with frequency are found. The changes in the mixing character of the modes are in most cases affected by the model mass and metallicity. Buoyancy glitches also have an impact on the mixing character. Significant fluctuations in the estimated coupling strength and period spacing are found for models approaching the luminosity bump, if the glitch impact of the frequencies is not considered in the applied asymptotic expansion.


2013 ◽  
Vol 462-463 ◽  
pp. 68-71
Author(s):  
Yu Ying Jiang ◽  
Qiang Liu

The measurement error models or EV(errors-in-variables) Models have been widely promoted in the field of statistics since 1877. According to the characteristics of the errors in variables, EV models can mainly be divided into three types: the additive model, the general measurement error model and berkson measurement error model. The emphases of researches in the EV models mainly focus on the effects of model estimation, hypothesis testing and model selection. In this paper, we concentrate on the research by conducted a systematic review of EV Models, in order to make a reference for researchers and practitioners.


1995 ◽  
Vol 15 (4) ◽  
pp. 355-366 ◽  
Author(s):  
J. J. Vanags ◽  
U. E. Viesturs ◽  
M. A. Priede

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