Universal resistive transition for two-dimensional superconductors

1981 ◽  
Vol 24 (11) ◽  
pp. 6758-6761 ◽  
Author(s):  
Petter Minnhagen
Keyword(s):  
Two Dimensional ◽  
Resistive Transition

Resistive transition in an extremely two-dimensional superconductor, α-(BEDT-TTF)2NH4Hg(SCN)4

1995 ◽  
Vol 70 (1-3) ◽  
pp. 915-916 ◽  
Author(s):  
Hirohiko Sato ◽  
Hiromi Taniguchi ◽  
Yasuhiro Nakazawa ◽  
Atsushi Kawamoto ◽  
Kiyonori Kato ◽  
...  
Keyword(s):  
Two Dimensional ◽  
Resistive Transition

Field-Induced Broadening of the Resistive Transition and Two-Dimensional Nature of Flux Pinning inY2Ba4Cu8O16Films

1990 ◽  
Vol 64 (14) ◽  
pp. 1666-1669 ◽  
Author(s):  
R. C. Budhani ◽  
D. O. Welch ◽  
M. Suenaga ◽  
R. L. Sabatini
Keyword(s):  
Flux Pinning ◽  
Two Dimensional ◽  
Resistive Transition

Resistive transition in two-dimensional arrays of superconducting weak links

1982 ◽  
Vol 26 (9) ◽  
pp. 5268-5271 ◽  
Author(s):  
David W. Abraham ◽  
C. J. Lobb ◽  
M. Tinkham ◽  
T. M. Klapwijk
Keyword(s):  
Weak Links ◽  
Two Dimensional ◽  
Resistive Transition

Periodic flux dependence of the resistive transition in two-dimensional superconducting arrays

1983 ◽  
Vol 28 (11) ◽  
pp. 6578-6581 ◽  
Author(s):  
M. Tinkham ◽  
David W. Abraham ◽  
C. J. Lobb
Keyword(s):  
Two Dimensional ◽  
Resistive Transition ◽  
Superconducting Arrays

Spectrophotometric measurements of objective-prism spectra

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler
Keyword(s):  
Progress Report ◽  
Two Dimensional ◽  
Objective Prism ◽  
Made In

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.

Introductory paper

1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan
Keyword(s):  
Line Intensity ◽  
Classification Scheme ◽  
Two Dimensional ◽  
Spectral Classification ◽  
Dimensional Array ◽  
Rr Lyrae ◽  
Metallic Line ◽  
Introductory Paper ◽  
Parameter Varying ◽  
Definition Of

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.

A one-dimensional self-gravitating stellar gas

1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar
Keyword(s):  
Gravitational Field ◽  
Phase Space ◽  
Motion Picture ◽  
Space Distribution ◽  
Two Dimensional ◽  
One Dimensional ◽  
Phase Space Distribution ◽  
Dimensional Phase Space ◽  
The Mean

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.

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