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- W111124328 abstract "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." @default.
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- W111124328 date "1958-01-01" @default.
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- W111124328 title "19. Astrophysical applications of selective magnetic rotation" @default.
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- W111124328 doi "https://doi.org/10.1017/s0074180900237753" @default.
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