Coherent optical polarization-shift-keying (POLSK) homodyne system using phase-diversity receivers

Author(s):  
I. Seto ◽  
T. Ohtsuki ◽  
H. Yshima ◽  
I. Sasase ◽  
S. Mori
1997 ◽  
Vol 45 (10) ◽  
pp. 1269-1279 ◽  
Author(s):  
S. Benedetto ◽  
R. Gaudino ◽  
P. Poggiolini

1995 ◽  
Vol 43 (2/3/4) ◽  
pp. 1603-1612 ◽  
Author(s):  
S. Benedetto ◽  
R. Gaudino ◽  
P. Poggiolini

2005 ◽  
Vol 252 (1-3) ◽  
pp. 162-166 ◽  
Author(s):  
Y.W. Song ◽  
Z. Pan ◽  
Y. Arieli ◽  
S.M.R. Motaghian ◽  
S.A. Havstad ◽  
...  

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


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