This morning I performed again the analysis after the shift of the input beam of the both WI and NI mirror images from the thermocamera (previous analysis can be found in #69785 and #69808, respectively). Here below are summarized the results:
WEST INPUT
Fig. 1 shows the thermocamera image of the WI.
Fig. 2 shows the output of the matlab code showing a new PA (or at least more visible now) w.r.t the last analysis after the beam shift.
Here there is a table summarizing the positions and information of the PAs:
| Element | Coordinate pixel [X, Y] | Offset from the center [cm] | Radial distance from the center [cm] | differential Temperature [degrees] |
| Center | [388, 241] | 0 | 0 | 0 |
| PA 1 | [384, 220] | [-0.54, -3.03] | 3.1 (upwards) | 0.8 |
| PA 2 | [382, 279] | [-0.85, 6] | 6.05 (downwards) | 0.4 |
NORTH INPUT
Fig. 3 shows the thermocamera image of the NI.
Fig. 4 shows the output of the MATLAB analysis, highlighting a PA that was not present in the images analyzed previously. The figure also shows a concentration of higher-temperature area near the center, with some peaks reaching approximately 0.3 °C.
Here there is a table summarizing the positions and information of the PAs:
| Element | Coordinate pixel [X, Y] | Offset from the center [cm] | Radial distance from the center [cm] | differential Temperature [degrees] |
| Center | [346, 204] | 0 | 0 | 0 |
| PA 1 | [310, 199] | [-5.73, -0.77] | 5.8 (leftwards) | 0.57 |
| PA 2 | [322, 197] | [-3.8, -1.07] | 3.95 (leftwards) | 0.35 |
Note:
The thermal contrast associated with a Point Absorber is obtained from the differential temperature map between the interferometer Lockedn (in CARM_NULL) and DOWN states. Measurements performed on different days can therefore exhibit some variability, even when the same Point Absorber is analysed.
This variability can arise from several contributions. The thermal background observed on the mirror is not completely uniform and can contain spatial structures related to thermal radiation reflected by the HR surface. These structures can change with the environmental and thermal conditions of the interferometer. In addition, the absolute temperature of the mirror and its surroundings, the thermal state and stability of the infrared camera, the transmission and optical properties of the ZnSe viewport, and small changes in the camera–mirror geometry can affect the measured temperature distribution.
The differential analysis reduces the effect of global temperature variations by aligning the median temperature of the mirror in the LOCKED and DOWN states. However, it does not completely remove changes in the spatial structure of the thermal background. Furthermore, the Point Absorber temperature is currently estimated from the maximum value within a local search region, making the result sensitive to local fluctuations and residual registration errors between the two images.
Consequently, variations of the measured Point Absorber thermal contrast, for example from approximately 0.65 °C to 0.8 °C (in the WI PA 1 case) in measurements performed on different days, should be interpreted primarily as a combination of the intrinsic thermal signal and the reproducibility/uncertainty of the measurement procedure.