Analysis of the birefringence of solid-core air-silica microstructured fibers

Author(s):  
Laurent Labonté ◽  
Elio Pone ◽  
Maksim Skorobogatiy ◽  
Nicolas Godbout ◽  
Suzanne Lacroix ◽  
...  
2010 ◽  
Vol 18 (10) ◽  
pp. 10731 ◽  
Author(s):  
Stéphane Virally ◽  
Nicolas Godbout ◽  
Suzanne Lacroix ◽  
Laurent Labonté

Author(s):  
Marco Antonio Cortez-Herrera ◽  
Diana Tentori

Due to its microstructure, photonic crystal fibers present wavelength regions with polarization-dependent loss, an aspect not observed in conventional fibers. We include this fact in their polarization characterization. In this research, the use of polarimetric methods to two different types of large-mode-area microstructured fibers has shown that both samples exhibited elliptical birefringence with residual torsion. We present the modifications required to perform the evaluation and justify its theoretical bases.


2007 ◽  
Vol 15 (2) ◽  
pp. 387 ◽  
Author(s):  
S. Laflamme ◽  
S. Lacroix ◽  
J. Bures ◽  
X. Daxhelet

1985 ◽  
Vol 30 (9) ◽  
pp. 711-711
Author(s):  
Steven C. Hayes

Author(s):  
R.S. Windeler ◽  
J.L. Wagener ◽  
D.J. DiGiovanni

2021 ◽  
pp. 1-1
Author(s):  
Olivier Vanvincq ◽  
Andy Cassez ◽  
Remi Habert ◽  
Hicham El Hamzaoui ◽  
Karen Baudelle ◽  
...  

2021 ◽  
pp. 1-1
Author(s):  
Alexis Dufour ◽  
Laure Bsawmaii ◽  
Damien Jamon ◽  
Emmanuel Marin ◽  
Sophie Neveu ◽  
...  

2018 ◽  
Vol 27 (1) ◽  
pp. 183-231 ◽  
Author(s):  
Pablo Cuartas-Restrepo

Abstract This work seeks to summarize some special aspects of a type of exoplanets known as super-Earths (SE), and the direct influence of these aspects in their habitability. Physical processes like the internal thermal evolution and the generation of a protective Planetary Magnetic Field (PMF) are directly related with habitability. Other aspects such as rotation and the formation of a solid core are fundamental when analyzing the possibilities that a SE would have to be habitable. This work analyzes the fundamental theoretical aspects on which the models of thermal evolution and the scaling laws of the planetary dynamos are based. These theoretical aspects allow to develop models of the magnetic evolution of the planets and the role played by the PMF in the protection of the atmosphere and the habitability of the planet.


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