|
Size: 562
Comment:
|
Size: 960
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 4: | Line 4: |
| == Polarimetry at the 30m telescope == | = Polarimetry at the 30m telescope = |
| Line 6: | Line 6: |
| === Documents === | == Documents == |
| Line 9: | Line 9: |
| [[attachment:thum_2008_xpol.pdf|Thum et al. 2008]], PASP, 120, 777 "" | [[attachment:thum_2008_xpol.pdf|Thum et al. 2008]], PASP, 120, 777 |
| Line 14: | Line 14: |
== Background material == * IAU definition of Stokes Parameters [[attachment:IAUdefs.pdf|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 [[attachment:bornWolf.pdf|Born & Wolf]] * The sign of Stokes V |
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
- The sign of Stokes V
