scholarly journals Integrated optical polarization-discriminating receiver in glass

1995 ◽  
Vol 13 (11) ◽  
pp. 2244-2249 ◽  
Author(s):  
D.L. Veasey ◽  
D.R. Larson
2000 ◽  
Vol 12 (10) ◽  
pp. 1358-1360 ◽  
Author(s):  
C. Pu ◽  
L.Y. Lin ◽  
E.L. Goldstein ◽  
N.J. Frigo ◽  
R.W. Tkach

2012 ◽  
Vol 748 (1) ◽  
pp. 17 ◽  
Author(s):  
Amy Jones ◽  
Lifan Wang ◽  
Kevin Krisciunas ◽  
Emily Freeland

2016 ◽  
Vol 34 (9) ◽  
pp. 2170-2174 ◽  
Author(s):  
Woo-Sung Chu ◽  
Sung-Moon Kim ◽  
Xiaoping Wu ◽  
Liu Wen ◽  
Min-Cheol Oh

1999 ◽  
Vol 38 (3) ◽  
pp. 530 ◽  
Author(s):  
Sang-Shin Lee ◽  
Sean Garner ◽  
William H. Steier ◽  
Sang-Yung Shin

2001 ◽  
Author(s):  
Hong Z. Hu ◽  
J. Chen ◽  
Haibin Zhang ◽  
Jisheng Yang ◽  
F. Geng

2012 ◽  
Vol 30 (17) ◽  
pp. 2884-2889 ◽  
Author(s):  
Jos J. G. M. van der Tol ◽  
Manuela Felicetti ◽  
Meint K. Smit

2000 ◽  
Vol 177 ◽  
pp. 315-318 ◽  
Author(s):  
Stefan J. Wagner ◽  
W. Seifert

AbstractWe investigate the polarization characteristics of optical emission from young pulsars. In a first attempt we search for polarization in images without time resolution in order to select suitable candidates for time-resolved studies. Polarization information constrains the nature of the faint optical emission of pulsars and will eventually allow to derive the topology of the field in those areas were optical radiation is emitted. We determine the polarization of the time-integrated optical emission of the SMC pulsar B0540-69 and the Vela pulsar B0833-45. We identify a new candidate optical counterpart for the young pulsar B1509-58 and find that the old candidate is unpolarized. The polarization of these three sources is rather high in view of the assumption that averaging over a putative swing of the polarization angle through 180 degrees will lead to depolarisation in the pulse-averaged signal.We also detect high degrees of polarization in the synchrotron nebula surrounding the LMC pulsar B0540-69, indicating even further similarity to the Crab.


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