Figures & data
Figure 1. Inverse results using N = 4 using errorless data: (a) temperature and (b) heat flux inverse predictions.
![Figure 1. Inverse results using N = 4 using errorless data: (a) temperature and (b) heat flux inverse predictions.](/cms/asset/9bf5156b-20c7-482f-a408-9e1c6b34ef0c/gipe_a_667093_f0001.gif)
Figure 2. Effect of the sampling rate on the inverse heat flux prediction with N = 7 using errorless data: (a) and (b)
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![Figure 2. Effect of the sampling rate on the inverse heat flux prediction with N = 7 using errorless data: (a) and (b) .](/cms/asset/a6602aed-9273-4a40-b047-871294830f1d/gipe_a_667093_f0002.gif)
Figure 3. Technique for estimating the noise present in the data: (a) first-order fit to data; (b) least-squares fit to residual; and (c) actual and estimated noises.
![Figure 3. Technique for estimating the noise present in the data: (a) first-order fit to data; (b) least-squares fit to residual; and (c) actual and estimated noises.](/cms/asset/e23d29d7-f913-49d6-92ed-8922e6826150/gipe_a_667093_f0003.gif)
Figure 4. Gaussian low-pass filter exploration: (a) optimum cut-off frequency range and (b) insensitivity of Gaussian filter to a small change in cut-off frequency.
![Figure 4. Gaussian low-pass filter exploration: (a) optimum cut-off frequency range and (b) insensitivity of Gaussian filter to a small change in cut-off frequency.](/cms/asset/ba6d5e8c-d117-4d14-9ab4-3a03edc1ac0f/gipe_a_667093_f0004.gif)
Figure 5. Inverse results using a normal distribution, with a standard deviation of 0.01 and a dimensionless cut-off frequency of 2.6: (a) noisy data used as input to the inverse code; (b) inverse temperature results and (c) inverse heat flux results.
![Figure 5. Inverse results using a normal distribution, with a standard deviation of 0.01 and a dimensionless cut-off frequency of 2.6: (a) noisy data used as input to the inverse code; (b) inverse temperature results and (c) inverse heat flux results.](/cms/asset/2cf8ce71-bf6d-4970-a0a0-2226cb87ca3f/gipe_a_667093_f0005.gif)
Figure 6. Temperature data for Beck triangle problem: (a) raw data with σ = 0.01 and (b) insensitivity of Gaussian filter to change in cut-off frequency.
![Figure 6. Temperature data for Beck triangle problem: (a) raw data with σ = 0.01 and (b) insensitivity of Gaussian filter to change in cut-off frequency.](/cms/asset/6398cef0-11ac-4dca-85e1-d2f951f93489/gipe_a_667093_f0006.gif)
Figure 7. Inverse results for the classical Beck triangle problem for: (a) surface temperature prediction and (b) surface heat flux prediction. Noise was simulated using a normal distribution, σ = 0.01 and used for regularization.
![Figure 7. Inverse results for the classical Beck triangle problem for: (a) surface temperature prediction and (b) surface heat flux prediction. Noise was simulated using a normal distribution, σ = 0.01 and used for regularization.](/cms/asset/d361c1d5-9910-4943-b6d6-9d4923a6c620/gipe_a_667093_f0007.gif)