Today, an analysis of the WI point absorber was performed using thermocamera images.
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Fig. 1 shows the reference thermal image selected for the analysis.
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Fig. 2 displays the MATLAB analysis output, highlighting a differential temperature of approximately 0.65 degrees for the point absorber (calculated by subtracting the mirror image in CARM_NULL from the image taken with the ITF in DOWN status).
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Fig. 3 illustrates the reconstructed mirror geometry, featuring the identified mirror center and the point absorber location based on pixel-to-distance mapping.
Geometric Mapping:
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X-Axis (Columns): The mirror center is located at column 388, whereas the point absorber is at column 384. This places the point absorber slightly to the left of the center (a offset of 3.5 pixels in the image, corresponding to approximately 0.5 cm in physical space).
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Y-Axis (Rows): The mirror center is located at row 241, whereas the point absorber is at row 221. This places the point absorber above the center (an offset of 19.5 pixels in the image, corresponding to approximately 3.0 cm in physical space).
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Radial Distance: The total estimated physical distance of the point absorber from the mirror center is approximately 3.1 cm.
Note that because this spatial mapping is reconstructed manually from off-axis thermocamera images, it is subject to geometric projection and pixel-resolution uncertainties. Consequently, this estimate should be considered less precise than the HWS measurement and serves primarily as a qualitative/cross-checking reference.
I will soon perform a similar analysis of the NI PAs.