High Resolution Program Flow Visualization of Hardware Accelerated Hybrid Multi-core Applications

2010 ◽  
Author(s):  
Daniel Hackenberg ◽  
Guido Juckeland ◽  
Holger Brunst
Keyword(s):  
High Resolution ◽  
Flow Visualization ◽  
Program Flow

scholarly journals Large scale flow visualization and anemometry applied to lab-on-a-chip models of porous media

Lab on a Chip ◽  
2016 ◽  
Vol 16 (15) ◽  
pp. 2851-2859 ◽  
Author(s):  
Johan Paiola ◽  
Harold Auradou ◽  
Hugues Bodiguel
Keyword(s):  
Porous Media ◽  
High Resolution ◽  
Velocity Field ◽  
Flow Visualization ◽  
Experimental Technique ◽  
Large Scale ◽  
Lab On A Chip ◽  
Large Scale Flow ◽  
Very High

The following is a report on an experimental technique that allows one to quantify and map the velocity field with very high resolution and simple equipment in large 2D devices.

High-resolution gas–oil two-phase flow visualization with a capacitance wire-mesh sensor

2010 ◽  
Vol 21 (3) ◽  
pp. 191-197 ◽  
Author(s):  
M.J. Da Silva ◽  
S. Thiele ◽  
L. Abdulkareem ◽  
B.J. Azzopardi ◽  
U. Hampel
Keyword(s):  
High Resolution ◽  
Flow Visualization ◽  
Two Phase Flow ◽  
Wire Mesh ◽  
Phase Flow ◽  
Gas Oil ◽  
Two Phase

Flow Textures: High-Resolution Flow Visualization

2005 ◽  
pp. 279-293 ◽  
Author(s):  
GORDON ERLEBACHER ◽  
BRUNO JOBARD ◽  
DANIEL WEISKOPF
Keyword(s):  
High Resolution ◽  
Flow Visualization

Observations of the spatial structure of interstellar hydrogen

1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles
Keyword(s):  
High Resolution ◽  
Spatial Structure ◽  
Velocity Dispersion ◽  
Temperature Variations

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.

Combining integrated systems-biology approaches with intervention-based experimental design provides a higher-resolution path forward for microbiome research

2019 ◽  
Vol 42 ◽  
Author(s):  
J. Alfredo Blakeley-Ruiz ◽  
Carlee S. McClintock ◽  
Ralph Lydic ◽  
Helen A. Baghdoyan ◽  
James J. Choo ◽  
...  
Keyword(s):  
Systems Biology ◽  
High Resolution ◽  
Experimental Design ◽  
Integrated Systems ◽  
Microbiome Research ◽  
Constructive Criticism

Abstract The Hooks et al. review of microbiota-gut-brain (MGB) literature provides a constructive criticism of the general approaches encompassing MGB research. This commentary extends their review by: (a) highlighting capabilities of advanced systems-biology “-omics” techniques for microbiome research and (b) recommending that combining these high-resolution techniques with intervention-based experimental design may be the path forward for future MGB research.

Very High Resolution Analysis of the Dynamics of a Coronal Plasmoid

1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker
Keyword(s):  
High Resolution ◽  
Solar Eclipse ◽  
Total Solar Eclipse ◽  
Field Of View ◽  
Small Field ◽  
High Resolution Analysis ◽  
Ccd Observations ◽  
Resolution Analysis ◽  
Very High ◽  
Small Field Of View

AbstractWe present the results of the analysis of a movie taken over a small field of view in the intermediate corona at a spatial resolution of 0.5“, a temporal resolution of 1 s and a spectral passband of 7 nm. These CCD observations were made at the prime focus of the 3.6 m aperture CFHT telescope during the 1991 total solar eclipse.

FeXIV Line Emission Polarization of the July 11, 1991 Solar Corona

1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož
Keyword(s):  
High Resolution ◽  
Solar Corona ◽  
Emission Line ◽  
Solar Eclipse ◽  
White Light ◽  
Preliminary Analysis ◽  
Line Emission ◽  
Total Solar Eclipse ◽  
Degree Of Polarization ◽  
High Resolution Images

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.

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