19. Astrophysical applications of selective magnetic rotation
1958 ◽
Vol 6
◽
pp. 166-168
Keyword(s):
When measuring the magnetic fields of sunspots the astronomer assumes that the magnetic field revealed by the inverse Zeeman effect is the same as if the splitting were produced by emission lines instead of absorption lines. No doubt this is in general a very fair approximation, but we have reason to remember sometimes that line absorption in the presence of magnetic fields is a very complicated process. In the immediate neighbourhood of absorption lines effects of magnetic rotation of the plane of polarization and magnetic double refraction may appear in the spectrum.
2013 ◽
Vol 9
(S302)
◽
pp. 385-388
◽
2016 ◽
Vol 12
(S325)
◽
pp. 59-62
Keyword(s):
Keyword(s):
1971 ◽
Vol 43
◽
pp. 3-23
◽
Keyword(s):
1971 ◽
Vol 43
◽
pp. 192-200
◽
Keyword(s):
2012 ◽
Vol 10
(H16)
◽
pp. 383-383
Keyword(s):
2013 ◽
Vol 9
(S302)
◽
pp. 130-133
Keyword(s):
2020 ◽
Vol 500
(1)
◽
pp. 153-176
1974 ◽
Vol 29
(5)
◽
pp. 786-796
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