The conventions for the polarization angle
arXiv:1612.03045 · doi:10.1007/s10686-016-9517-y
Abstract
Since more than a century astronomers measure the position angle of the major axis of the polarization ellipse starting from the North direction and increasing counter-clockwise, when looking at the source. This convention has been enforced by the IAU with a Resolution in 1973. Much later the WMAP satellite, which has observed the polarization of the cosmic microwave background, has unfortunately adopted the opposite convention: the polarization position angle is measured starting from the South and increasing clockwise, when looking at the source. This opposite convention has been followed by most cosmic microwave background polarization experiments and is causing obvious problems and misunderstandings. The attempts and prospects to enforce the official IAU convention are described.
Accepted for publication in Experimental Astronomy
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- Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization
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- The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II
- Impact of half-wave plate systematics on the measurement of CMB -mode polarization
- Optical Polarimetry of the May 2022 Lunar Eclipse
- Detection of polarized Fermi-bubble synchrotron and dust emission