A simple and efficient strategy for solving very large-scale generalized cable-trench problems

Networks ◽  
2015 ◽  
Vol 67 (3) ◽  
pp. 199-208 ◽  
Author(s):  
Francis J. Vasko ◽  
Eric Landquist ◽  
Gregory Kresge ◽  
Adam Tal ◽  
Yifeng Jiang ◽  
...  
2019 ◽  
Vol 166 ◽  
pp. 265-275 ◽  
Author(s):  
Xiaodong Liu ◽  
Julien Réthoré ◽  
Marie-Christine Baietto ◽  
Philippe Sainsot ◽  
Antonius Adrianus Lubrecht

1994 ◽  
Vol 1 (1) ◽  
pp. 25-30 ◽  
Author(s):  
John X. He ◽  
Wayne L. Cody ◽  
Annette M. Doherty

2017 ◽  
Vol 180 ◽  
pp. 1160-1169 ◽  
Author(s):  
Francesco Pittau ◽  
Laura E. Malighetti ◽  
Giuliana Iannaccone ◽  
Gabriele Masera

2015 ◽  
Vol 13 (19) ◽  
pp. 5520-5531 ◽  
Author(s):  
Sandy Desrat ◽  
Camille Remeur ◽  
Fanny Roussi

The synthesis, on a large scale, with very good yield and er via an efficient strategy, of a chiral 4-substituted 2-cyclohexenone intermediate, was a milestone in the synthesis of seven analogues of meiogynin A, a natural sesquiterpenoid dimer.


2020 ◽  
Vol 106 ◽  
pp. 102192 ◽  
Author(s):  
Ahmad Mohamad Mezher ◽  
Pedro Enrique Iturria Rivera ◽  
Julián Cárdenas-Barrera ◽  
Julian Meng ◽  
Eduardo Castillo Guerra

2018 ◽  
Author(s):  
Chongyuan Luo ◽  
Angeline Rivkin ◽  
Jingtian Zhou ◽  
Justin P. Sandoval ◽  
Laurie Kurihara ◽  
...  

Single-cell DNA methylome profiling has enabled the study of epigenomic heterogeneity in complex tissues and during cellular reprogramming. However, broader applications of the method have been impeded by the modest quality of sequencing libraries. Here we report snmC-seq2, which provides improved read mapping, reduced artifactual reads, enhanced throughput, as well as increased library complexity and coverage uniformity compared to snmC-seq. snmC-seq2 is an efficient strategy suited for large scale single-cell epigenomic studies.


1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.


1994 ◽  
Vol 144 ◽  
pp. 29-33
Author(s):  
P. Ambrož

AbstractThe large-scale coronal structures observed during the sporadically visible solar eclipses were compared with the numerically extrapolated field-line structures of coronal magnetic field. A characteristic relationship between the observed structures of coronal plasma and the magnetic field line configurations was determined. The long-term evolution of large scale coronal structures inferred from photospheric magnetic observations in the course of 11- and 22-year solar cycles is described.Some known parameters, such as the source surface radius, or coronal rotation rate are discussed and actually interpreted. A relation between the large-scale photospheric magnetic field evolution and the coronal structure rearrangement is demonstrated.


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