scholarly journals MARVEL analysis of the high-resolution rovibrational spectra of H16O35Cl

2021 ◽  
pp. 111561
Author(s):  
Balázs Rácsai ◽  
Tibor Furtenbacher ◽  
Luciano Fusina ◽  
Gianfranco Di Lonardo ◽  
Attila G. Császár
Author(s):  
Katy L. Chubb ◽  
Olga Naumenko ◽  
Stefan Keely ◽  
Sebestiano Bartolotto ◽  
Skye Macdonald ◽  
...  

Author(s):  
Katy L. Chubb ◽  
Megan Joseph ◽  
Jack Franklin ◽  
Naail Choudhury ◽  
Tibor Furtenbacher ◽  
...  

2004 ◽  
Vol 5 (2) ◽  
pp. 189-199 ◽  
Author(s):  
Vladimir G. Tyuterev ◽  
Laurence Régalia-Jarlot ◽  
David W. Schwenke ◽  
Sergei A. Tashkun ◽  
Yurii G. Borkov

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.


1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

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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