Fourier-space image processing for spherical experiments on OMEGA (invited)

2001 ◽  
Vol 72 (1) ◽  
pp. 635-642 ◽  
Author(s):  
V. A. Smalyuk ◽  
T. R. Boehly ◽  
L. S. Iwan ◽  
T. J. Kessler ◽  
J. P. Knauer ◽  
...  
Author(s):  
Jūratė Sužiedelytė Visockienė ◽  
Eglė Tumelienė ◽  
Ignas Daugėla ◽  
Jūratė Kučienė
Keyword(s):  

2018 ◽  
Author(s):  
Julio Sanchez ◽  
Maria P. Canton ◽  
William Perrizo
Keyword(s):  

1993 ◽  
Vol 32 (32) ◽  
pp. 6556 ◽  
Author(s):  
S. Woolven ◽  
V. M. Ristic ◽  
P. Chevrette

2004 ◽  
Vol 37 (5) ◽  
pp. 716-723
Author(s):  
M. Laridjani ◽  
F. Dénoyer

One of the key obstacles in the progress of certain aspects of solid-state physics is the determination of the nature of irregularities in the atomic network of matter and their correlation with macroscopic properties. In this work, an original structural result is presented, namely the presence of icosahedral clusters in an Al solid solution, as deduced from the analysis of the total Fourier-space image. This work has led to the belief that these non-crystalline clusters create a fundamental irregularity in the network of a non-ideal solid solution.


Nano Letters ◽  
2020 ◽  
Vol 20 (10) ◽  
pp. 7463-7468 ◽  
Author(s):  
Ningbin Mao ◽  
Junhong Deng ◽  
Xuecai Zhang ◽  
Yutao Tang ◽  
Mingke Jin ◽  
...  

Author(s):  
Ali Nekouzadeh ◽  
Guy M. Genin

Quantification of changes in the total length of randomly oriented and possibly curved lines appearing in an image is a necessity in a wide variety of biological applications. Here, we present an automated approach based upon Fourier space analysis. Scaled, band-pass filtered power spectral densities of greyscale images are integrated to provide a quantitative measurement of the total length of lines of a particular range of thicknesses appearing in an image. A procedure is presented to correct for changes in image intensity. The method is most accurate for two-dimensional processes with fibres that do not occlude one another.


1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.


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