Recent comparisons of magnetic field directions derived from maser Zeeman splitting with those derived from continuum source rotation measures have prompted new analysis of the propagation of the Zeeman split components, and the inferred field orientation. In order to do this, we first review differing electric field polarization conventions used in past studies. With these clearly and consistently defined, we then show that for a given Zeeman splitting spectrum, the magnetic field direction is fully determined and predictable on theoretical grounds: When a magnetic field is oriented away from the observer, the left-hand circular polarization is observed at higher frequency and the right-hand polarization at lower frequency. This is consistent with classical Lorentzian derivations. The consequent interpretation of recent measurements then raises the possibility of a reversal between the large-scale field (traced by rotation measures) and the small-scale field (traced by maser Zeeman splitting). © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
CITATION STYLE
Green, J. A., Gray, M. D., Robishaw, T., Caswell, J. L., & Mcclure-Griffiths, N. M. (2014). A quantum mechanical approach to establishing the magnetic field orientation from a maser zeeman profile. Monthly Notices of the Royal Astronomical Society, 440(4), 2988–2996. https://doi.org/10.1093/mnras/stu429
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