The Production of Rotation Measure Gradients in the Lobes of Extragalactic Radio Sources
1990 ◽
Vol 140
◽
pp. 477-481
Keyword(s):
Cygnus A
◽
It is proposed that the large rotation measure gradients observed in the lobes of some extragalactic radio sources are produced by non–linear Kelvin–Helmholtz surface waves. Related small scale turbulence is responsible for a “diffuse spray” of relativistic plasma and magnetic field into the surrounding medium. The mixture of magnetic field and thermal plasma causes large rotation measure variations on the scale of the Kelvin–Helmholtz waves. An order of magnitude prediction of the effect is in good agreement with the observations of Cygnus A and PKS 2104–25 N.
1990 ◽
Vol 140
◽
pp. 472-472
Keyword(s):
1985 ◽
Vol 106
◽
pp. 251-252
Keyword(s):
1990 ◽
Vol 140
◽
pp. 55-58
Keyword(s):
1988 ◽
Vol 101
◽
pp. 355-358
Keyword(s):
1997 ◽
Vol 166
◽
pp. 215-218
1987 ◽
Vol 37
(2)
◽
pp. 299-321
◽
Keyword(s):
2021 ◽
pp. 470-477
2015 ◽
Vol 2
(1)
◽
pp. 329-359