Changes between Version 6 and Version 7 of docs/CommissioningPlan/P3.7


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Timestamp:
04/22/22 20:47:47 (3 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan/P3.7

    v6 v7  
    1 == P3.7 Checking field-stabilized mode/bearing rotation service ==
     1== P3.7 Internal TT loop working and performance==
    22 
    33- **Phase**             :       3 
    44- **Status**            :       Draft   
    5 - **Category**  :       Nighttime testing (functionality and operability) (C5)
     5- **Category**  :       Nighttime testing (functionality and operability) (C5) + Nighttime testing for performance (C7)
    66- **Recurrence**        :       once at commissioning
    7 - **Duration**  :       2 hours
     7- **Duration**  :       3 hours
    88
    99**Description**
    10 - The field stabilized mode, or in other words, the working of the bearing tracking service, will be tested.
     10- Evaluate the performance of the internal tip-tilt (TT) loop of SHARK-NIR for stars of varying brightness.
    1111
    1212**Prerequisites**
    13 - Atmospheric conditions: AO working conditions.
     13- Atmospheric conditions: TBD
    1414- Authorize SHARK-NIR on the SX side.
    15 - Targets (star cluster) near zenith and horizon (say airmass of 2).
     15- Stars (of known brightness from 8mag-13mag in the R band) as targets.
     16- AO is working.
    1617
    1718**Procedure**
    18 - Select the target near airmass 2. There should be stars spread across the entire SCICAM, preferably close to the edges as well.
    19 - Start the bearing tracking services (field-stabilized mode).
    20 - Take short-exposure images for a duration of ##minutes.
    21 - Check the positions of these stars.
    22 - Repeat the same for the target close to the zenith.
    23 - Repeat the same steps for a target where the rotation of the bearing is in the opposite direction.
     19- Run the internal TT loop after the star is acquired and the AO loop is closed.
     20- Take unsaturated images of the star for a given (?) science filter before and after the internal TT loop closure in the SCICAM.
     21- Take data in TECCAM simultaneously.
     22- Use data to estimate the improvement of the residual jitter after the TT loop is closed.
     23- Repeat for different star magnitudes.
     24- should we perform as a function of elevation as well? We can choose stars accordingly, then?
    2425
    2526**Templates**
     27- SHARKNIR_gen_tiptilt_loop (not released)
    2628
    2729**Success criteria**
    28 - The bearing tracking service works well, and the field is stabilized within the precision needed.
     30- Estimate the residual jitter after SOUL-AO is closed for a given seeing and star brightness.
     31- Checking the working and performance of the internal TT loop.
     32- Quantify and numbers to add?
    2933
    3034**Notes**