Single mode, visible white-light supercontinuum in normally dispersive fiber

Author(s):  
P. A. Champert ◽  
V. Couderc ◽  
S. Février ◽  
P. Leproux ◽  
P. Nérin ◽  
...  
Author(s):  
Stéphane Coen ◽  
Alvin Hing Lun Chau ◽  
Rainer Leonhardt ◽  
John D. Harvey ◽  
Jonathan C. Knight ◽  
...  

Author(s):  
P. A. Champert ◽  
V. Couderc ◽  
L. Grossard ◽  
C. Froehly ◽  
A. Barthélémy ◽  
...  

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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