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If the fast steering mirror is too slow, it will not be able to stabilize image jitter.
Risk Effects:
If we cannot correct for image motion, then science images will be blurred, reducing the coronagraphic contrast and limiting which GMagAO-X science can be performed.
Risk Assessment:
Risk Ratings
Likelihood
Consequence
Initial
3
4
Current
3
4
Target
1
2
Initial Risk Notes:
The FSM pupil is currently designed to be 16mm in diameter.
Risk Notes/Updates:
Cost Impacts:
Estimated cost if risk is realized:
Explanation for cost risk:
Risk mitigation list:
Light-weight FSM mirror
Develop custom control electronics to operate the FSM faster
[ ]
[ ]
The text was updated successfully, but these errors were encountered:
Risk creation date: 2/2/2024
Last Modified: 2/2/2024
Risk type: Technical
Risk Approach: Mitigate
Risk Owner: Doug Kelly
Risk Statement:
If the fast steering mirror is too slow, it will not be able to stabilize image jitter.
Risk Effects:
If we cannot correct for image motion, then science images will be blurred, reducing the coronagraphic contrast and limiting which GMagAO-X science can be performed.
Risk Assessment:
Initial Risk Notes:
The FSM pupil is currently designed to be 16mm in diameter.
Risk Notes/Updates:
Cost Impacts:
Estimated cost if risk is realized:
Explanation for cost risk:
Risk mitigation list:
Light-weight FSM mirror
Develop custom control electronics to operate the FSM faster
[ ]
[ ]
The text was updated successfully, but these errors were encountered: