Changes between Version 6 and Version 7 of docs/CommissioningPlan/P3.17
- Timestamp:
- 03/03/23 14:11:19 (21 months ago)
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docs/CommissioningPlan/P3.17
v6 v7 1 == P3.17 Orient the coronagraphs ==1 == P3.17 Orient the apodizers == 2 2 3 3 - **Phase** : 3 4 4 - **Status** : Draft 5 5 - **Category** : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6) 6 - **Recurrence** : before every observing target (CI, LSS), starting from commissioning.6 - **Recurrence** : before every observing target (CI, eventually LSS?), starting from commissioning. 7 7 - **Duration** : 4 hours 8 8 9 9 **Description** 10 - Adjust the orientation of the coronagraphic masks with respect to the true orientation of the M2 spider by rotating the SHARK-NIR derotator.10 - Adjust the orientation of the Shaped Pupil apodizers with respect to the true orientation of the M2 spider by rotating the SHARK-NIR derotator. 11 11 12 12 **Prerequisites** … … 16 16 17 17 **Procedure** 18 - Pointing to a star, the first coronagraph is inserted in the path. The bearing is rotated, maximizing the contrast achieved on the SCICAM. (use the pupil lens to see the pupil's alignment, maybe)?19 - This operation is repeated for all the coronagraphs.18 - Insert the first apodizer in the path and measure its orientation on SCICAM illuminating it with the internal fiber. Then point a star, remove the apodizer and measure the orientation of the M2 spider on SCICAM. Rotate the bearing by the delta between the two orientations. Iterarate, if necessary, until delta is below 0.5deg. 19 - This operation is repeated for the other two apodizers. 20 20 21 21 **Templates** … … 23 23 24 24 **Success criteria** 25 - All the coronagraphs are aligned to the true orientation of the M2 spider by m aximizing the contrast atSCICAM.25 - All the coronagraphs are aligned to the true orientation of the M2 spider by minimizing the differential orientation on SCICAM. 26 26 - Note down the contrast achieved for all the coronagraphs, including the atmospheric conditions and the brightness of the on-axis star. 27 27