A quantum mechanical approach to establishing the magnetic field orientation from a maser Zeeman profile

被引:7
作者
Green, J. A. [1 ,2 ]
Gray, M. D. [3 ]
Robishaw, T. [4 ]
Caswell, J. L. [2 ]
McClure-Griffiths, N. M. [2 ]
机构
[1] Jodrell Bank Observ, SKA Org, Macclesfield SK11 9DL, Cheshire, England
[2] Australia Telescope Natl Facil, CSIRO Astron & Space Sci, Epping, NSW 1710, Australia
[3] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England
[4] Natl Res Council Canada, Herzberg Astron & Astrophys Programs, Domin Radio Astrophys Observ, Penticton, BC V2A 6J9, Canada
关键词
magnetic fields; masers; polarization; radiative transfer; STAR-FORMING-REGIONS; CIRCULAR-POLARIZATION; ASTROPHYSICAL MASERS; OH MASERS; RADIATION; AMPLIFICATION; EMISSION; CLOUDS; LINE;
D O I
10.1093/mnras/stu429
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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).
引用
收藏
页码:2988 / 2996
页数:9
相关论文
共 49 条
[1]   THE SOLAR MAGNETOGRAPH [J].
BABCOCK, HW .
ASTROPHYSICAL JOURNAL, 1953, 118 (03) :387-&
[2]   REPORTS ON THE PROGRESS OF ASTRONOMY - GENERAL MAGNETIC FIELDS IN THE SUN AND STARS [J].
BABCOCK, HW ;
COWLING, TG .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1953, 113 (03) :357-381
[3]  
Boas ML., 1966, Mathematical Methods in Physical Sciences
[4]   Rotation measures of extragalactic sources behind the southern Galactic plane: New insights into the large-scale magnetic field of the inner Milky Way [J].
Brown, J. C. ;
Haverkorn, M. ;
Gaensler, B. M. ;
Taylor, A. R. ;
Bizunok, N. S. ;
McClure-Griffiths, N. M. ;
Dickey, J. M. ;
Green, A. J. .
ASTROPHYSICAL JOURNAL, 2007, 663 (01) :258-266
[5]  
Davies R. D., 1974, P IAU S, V60, P275
[6]   MEASUREMENT OF MAGNETIC FIELDS IN INTERSTELLAR CLOUDS [J].
DAVIES, RD ;
VERSCHUUR, GL ;
WILD, PAT .
NATURE, 1962, 196 (4854) :563-&
[7]   LINEARLY POLARIZED RADIATION FROM ASTROPHYSICAL MASERS DUE TO MAGNETIC-FIELDS WHEN THE RATE FOR STIMULATED-EMISSION EXCEEDS THE ZEEMAN FREQUENCY [J].
DEGUCHI, S ;
WATSON, WD .
ASTROPHYSICAL JOURNAL, 1990, 354 (02) :649-659
[8]  
Edmonds A R, 1996, PRINCETON LANDMARKS
[9]  
Eisberg R., 1974, Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles
[10]   POLARIZATION OF ASTRONOMICAL MASER RADIATION [J].
ELITZUR, M .
ASTROPHYSICAL JOURNAL, 1991, 370 (01) :407-418