KAGRA MIR (General)
MarcEisenmann - 18:17, Wednesday 09 February 2022 (2835)
Further check of power fluctuations

Katsuki, Marc

For the measurement with 30 deg input polarization angle we swapped the scan and shift directions (ie in the attached figures 2 nearby points in Y are close in time).

We can now see the stripes in the horizontal direction.

This confirms that the power fluctuations are not correlated to the mirror position.

Images attached to this report
2835_20220209101722_shinkosha7horizontalscan.png