IRISPOLReduce IRIS imaging polarimetry data.
Reduce IRIS imaging polarimetry data.
IRISPOL reduces data obtained with the AATIRIS polarimeter using the wolaston prism poarizer. The
data for a single observation consists of four Figaro files containing the frames for plate position 0, 45,
22.5 and 67.5 degrees. Within each frame are selected two images corresponding to the O and E rays
for a siingle mask slot. These spectra are combined to derive a polarization image in TSP
format.
Two different algorithms may be selected for the polarimetry reduction. The two algorithms differ in the method used to compensate for transparency variations between the observations at the two plate positions.
The variances on the polarization data are calculated from photon statistics plus readout noise.
| 1 | POS1 | Char | The Figaro data file for position 0.0. |
| 2 | POS2 | Char | The Figaro data file for position 45.0. |
| 3 | POS3 | Char | The Figaro data file for position 22.5. |
| 4 | POS4 | Char | The Figaro data file for position 67.5. |
X1 | Integer | X coordinate of the bottom left corner of block |
|
Y1 | Integer | Y coordinate of the bottom left corner of block |
|
WIDTH | Integer | Width of the block |
|
HEIGHT | Integer | Height of the block |
|
XSEP | Integer |
|
|
YSEP | Integer |
|
|
ALGORITHM | Char | The Algorithm to use for stokes parameter
calculation ( |
|
OUTPUT | TSP, 1D | The Output dataset. |
3/5/1993