|
Size: 960
Comment:
|
Size: 979
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 9: | Line 9: |
| [[attachment:thum_2008_xpol.pdf|Thum et al. 2008]], PASP, 120, 777 * Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments |
[[attachment:thum_2008_xpol.pdf|Thum et al. 2008]], PASP, 120, 777 * Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments |
| Line 13: | Line 13: |
| [[attachment:wiesemeyer-2010-polarimetry-v3.pdf|Wiesemeyer, Thum 2010, IRAM Report]] | [[attachment:wiesemeyer-2010-polarimetry-v3.pdf|Wiesemeyer & Thum 2010, IRAM Report]] |
| Line 19: | Line 19: |
| Radioastronomy, including the 30m telescope, uses these definitions. Note however that according | Radioastronomy, including the 30m telescope, uses these definitions. Note however that according |
| Line 21: | Line 21: |
| by [[attachment:bornWolf.pdf|Born & Wolf]] | by [[attachment:bornWolf.pdf|Born & Wolf in "Classical Optics"]] |
Polarimetry at the 30m telescope
Documents
- XPOL—the Correlation Polarimeter at the IRAM 30-m Telescope
Thum et al. 2008, PASP, 120, 777
- Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments
- Polarimetry with EMIR/XPOL - commisioning report (August 2010)
Background material
- IAU definition of Stokes Parameters
They are found here. Radioastronomy, including the 30m telescope, uses these definitions. Note however that according to this definition the sign of Stokes V is opposite to the convention in classical optics as described by Born & Wolf in "Classical Optics"
- The sign of Stokes V