scholarly journals Mechanically stretched chromosomes as targets for high-resolution FISH mapping.

1995 ◽  
Vol 5 (1) ◽  
pp. 13-20 ◽  
Author(s):  
M Laan ◽  
O P Kallioniemi ◽  
E Hellsten ◽  
K Alitalo ◽  
L Peltonen ◽  
...  
Keyword(s):  
High Resolution ◽  
Fish Mapping

High-resolution FISH mapping of the rat α 2u -globulin multigene family

2000 ◽  
Vol 11 (4) ◽  
pp. 292-299 ◽  
Author(s):  
D.A. McFadyen ◽  
J. Locke
Keyword(s):  
High Resolution ◽  
Multigene Family ◽  
Fish Mapping

High-resolution FISH mapping of β-defensin genes to river buffalo and sheep chromosomes suggests a chromosome discrepancy in cattle standard karyotypes

1996 ◽  
Vol 75 (1) ◽  
pp. 10-13 ◽  
Author(s):  
L. lannuzzi ◽  
D.S. Gallagher ◽  
G.P. Di Meo ◽  
G. Diamond ◽  
C.L. Bevins ◽  
...  
Keyword(s):  
High Resolution ◽  
River Buffalo ◽  
Fish Mapping

scholarly journals A high-resolution cat radiation hybrid and integrated FISH mapping resource for phylogenomic studies across Felidae

Genomics ◽  
2009 ◽  
Vol 93 (4) ◽  
pp. 299-304 ◽  
Author(s):  
Brian W. Davis ◽  
Terje Raudsepp ◽  
Alison J. Pearks Wilkerson ◽  
Richa Agarwala ◽  
Alejandro A. Schäffer ◽  
...  
Keyword(s):  
High Resolution ◽  
Radiation Hybrid ◽  
Fish Mapping ◽  
Mapping Resource

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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