scholarly journals Leveraging scatter in two-dimensional spectroscopy: passive phase drift correction enables a global phasing protocol

2020 ◽  
Vol 28 (22) ◽  
pp. 32869
Author(s):  
Lawson T. Lloyd ◽  
Ryan E. Wood ◽  
Marco A. Allodi ◽  
Siddhartha Sohoni ◽  
Jacob S. Higgins ◽  
...  
Keyword(s):  
Two Dimensional ◽  
Drift Correction ◽  
Phase Drift ◽  
Passive Phase

scholarly journals Quantitative MR thermometry based on phase-drift correction PRF shift method at 0.35 T

2018 ◽  
Vol 17 (1) ◽  
Author(s):  
Yuping Chen ◽  
Mengke Ge ◽  
Rizwan Ali ◽  
Hejun Jiang ◽  
Xiaoyan Huang ◽  
...  
Keyword(s):  
Mr Thermometry ◽  
Drift Correction ◽  
Shift Method ◽  
Phase Drift ◽  
Quantitative Mr

On-Line Thévenin Impedance Estimation Based on PMU Data and Phase Drift Correction

2018 ◽  
Vol 9 (2) ◽  
pp. 1033-1042 ◽  
Author(s):  
Bahman Alinezhad ◽  
Hossein Kazemi Karegar
Keyword(s):  
Drift Correction ◽  
Phase Drift ◽  
On Line

scholarly journals The importance of phase drift correction for accurate MR thermometry in long duration MR-HIFU exposures

2015 ◽  
Vol 3 (S1) ◽  
Author(s):  
Chenchen Bing ◽  
Charles Mougenot ◽  
Robert Staruch ◽  
Elizabeth Ramsay ◽  
Alain Schmitt ◽  
...  
Keyword(s):  
Mr Thermometry ◽  
Drift Correction ◽  
Phase Drift ◽  
Long Duration

Passively correcting phase drift in two-dimensional infrared spectroscopy

2006 ◽  
Vol 31 (19) ◽  
pp. 2918 ◽  
Author(s):  
Feng Ding ◽  
Prabuddha Mukherjee ◽  
Martin T. Zanni
Keyword(s):  
Infrared Spectroscopy ◽  
Two Dimensional ◽  
Phase Drift ◽  
Two Dimensional Infrared Spectroscopy

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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