Effect of Faraday Rotation on the Circular Polarization of the Crab Nebula

1974 ◽  
Vol 189 ◽  
pp. 249
Author(s):  
Michael J. Gerver
Solar Physics ◽  
1976 ◽  
Vol 50 (2) ◽  
pp. 465-480 ◽  
Author(s):  
Y. Sofue ◽  
K. Kawabata ◽  
F. Takahashi ◽  
N. Kawajiri

1973 ◽  
Vol 52 ◽  
pp. 169-179
Author(s):  
P. G. Martin ◽  
R. Illing ◽  
J. R. P. Angel

A search in many small regions of the Crab Nebula has resulted in the detection of a small component of circular polarization. The variation of the sign and magnitude with position in the Nebula indicates that the polarization is of interstellar origin. On the basis of the polarity, strength, and colour dependence, it is concluded that the composition of the aligned grains causing this polarization is dielectric. Metallic particles are clearly ruled out.


1971 ◽  
Vol 46 ◽  
pp. 118-118
Author(s):  
R. N. Manchester

During April, 1970, the 300-ft telescope of the National Radio Astronomy Observatory was used to determine the mean polarisation of the Crab Nebula pulsar radiation at several frequencies around 400 MHz. The position angle of the highly polarised precursor measured at each frequency, corrected for ionospheric Faraday rotation and plotted against inverse frequency squared is shown in Figure 1. The observed variation of the position angle with frequency is consistent with Faraday rotation of the plane of polarisation with a rotation measure of −40.5 ± 4.5 rad/m2. This value is of the same sign but larger than the rotation measure for the nebular radiation in the vicinity of the pulsar.


1991 ◽  
Vol 368 ◽  
pp. 231 ◽  
Author(s):  
Michael F. Bietenholz ◽  
Philipp P. Kronberg

2011 ◽  
Vol 528 ◽  
pp. A11 ◽  
Author(s):  
H. Wiesemeyer ◽  
C. Thum ◽  
D. Morris ◽  
J. Aumont ◽  
C. Rosset

Nature ◽  
1971 ◽  
Vol 230 (5289) ◽  
pp. 103-103 ◽  
Author(s):  
J. D. LANDSTREET ◽  
J. R. P. ANGEL

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