7.3: High-Luminance Ultra-High-Resolution PDPs with Twin-Path Coplanar Discharge Cells

2009 ◽  
Vol 40 (1) ◽  
pp. 62
Author(s):  
Yoshikuni Hirano ◽  
Keiji Ishii ◽  
Takenobu Usui ◽  
Yukio Murakami
2003 ◽  
Author(s):  
Gang Yang ◽  
Jianbo Cheng ◽  
Zulun Lin ◽  
Qionghua Wang ◽  
Wenbing Chen

1998 ◽  
Author(s):  
Jianbo Cheng ◽  
Jun Wang ◽  
Zhenxiang Cheng ◽  
Kangcheng Qi ◽  
Min Zhou

1999 ◽  
Vol 7 (3) ◽  
pp. 183 ◽  
Author(s):  
Qionghua Wang ◽  
Jianbo Cheng ◽  
Zulun Lin ◽  
Gang Yang

1998 ◽  
Author(s):  
Jianbo Cheng ◽  
Zexiang Chen ◽  
Guichuan Cao ◽  
Jun Wang ◽  
Kangcheng Qi

1996 ◽  
Vol 36 (16) ◽  
pp. 2575-2578
Author(s):  
ALLEN B POIRSON ◽  
LAURENCE T MALONEY

2002 ◽  
Vol 33 (1) ◽  
pp. 1084 ◽  
Author(s):  
Jianbo Cheng ◽  
Qiong-Hua Wang ◽  
Zulun Lin

1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

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.


2019 ◽  
Vol 42 ◽  
Author(s):  
J. Alfredo Blakeley-Ruiz ◽  
Carlee S. McClintock ◽  
Ralph Lydic ◽  
Helen A. Baghdoyan ◽  
James J. Choo ◽  
...  

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.


1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker

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.


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