Analysis of the two-dimensional turbulence in pure electron plasmas by means of advanced statistical techniques

Author(s):  
M. Romé ◽  
F. Lepreti ◽  
G. Maero ◽  
R. Pozzoli ◽  
A. Vecchio ◽  
...  
2013 ◽  
Vol 87 (6) ◽  
Author(s):  
F. Lepreti ◽  
M. Romé ◽  
G. Maero ◽  
B. Paroli ◽  
R. Pozzoli ◽  
...  

2005 ◽  
Vol 26 (4) ◽  
pp. 185-193 ◽  
Author(s):  
Andreas Hinz ◽  
Elmar Brähler ◽  
Peter Schmidt ◽  
Cornelia Albani

Abstract. The Portrait Values Questionnaire (PVQ) comprises 10 basic values that guide behavior. The Schwartz model postulates that these 10 values build a circumplex structure. We examined the PVQ with respect to its dimensional structure using a representative sample (N = 1896) of the German population. The results of three widely used analyses were compared: multidimensional scaling, factorial analysis (with varimax rotation) of raw scores, and factorial analysis with ipsative values. Furthermore, rank correlations between the theoretically assumed circular distances and the empirical data were calculated. The analyses confirmed that the 10 dimensions of the PVQ can be depicted in a two-dimensional plane. However, the statistical techniques chosen yielded different arrangements of the 10 values in the plane. All statistical methods failed to confirm the circumplex structure postulated by Schwartz. Nevertheless, dimensions of higher order that condense the 10 dimensions can be derived for applications of the PVQ.


2018 ◽  
Vol 848 ◽  
pp. 256-287 ◽  
Author(s):  
N. C. Hurst ◽  
J. R. Danielson ◽  
D. H. E. Dubin ◽  
C. M. Surko

The dynamics of two-dimensional (2-D) ideal fluid vortices is studied experimentally in the presence of an irrotational strain flow. Laboratory experiments are conducted using strongly magnetized pure electron plasmas, a technique which is made possible by the isomorphism between the drift–Poisson equations describing plasma dynamics transverse to the field and the 2-D Euler equations describing an ideal fluid. The electron plasma system provides an excellent opportunity to study the dynamics of a 2-D Euler fluid due to weak dissipation and weak 3-D effects, simple diagnosis and precise control. The plasma confinement apparatus used here was designed specifically to study vortex dynamics under the influence of external flow by applying boundary conditions in two dimensions. Additionally, vortex-in-cell simulations are carried out to complement the experimental results and to extend the parameter range of the studies. It is shown that the global dynamics of a quasi-flat vorticity profile is in good quantitative agreement with the theory of a piecewise-constant elliptical patch of vorticity, including the equilibria, dynamical orbits and stability properties. Deviations from the elliptical patch theory are observed for non-flat vorticity profiles; they include inviscid damping of the orbits and modified stability limits. The dependence of these phenomena on the flatness of the initial profile is discussed. The relationship of these results to other theoretical, numerical and experimental studies is also discussed.


2008 ◽  
Vol 15 (4) ◽  
pp. 042312
Author(s):  
Dastgeer Shaikh ◽  
P. K. Shukla

2018 ◽  
Author(s):  
Shohei Yamada ◽  
Haruhiko Himura ◽  
Toshiki Kato ◽  
Shigehumi Okada ◽  
Akio Sanpei ◽  
...  

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


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