# SPDX-License-Identifier: BSD-2-Clause # # Copyright (C) 2019, Raspberry Pi Ltd # # ctt_noise.py - camera tuning tool noise calibration from ctt_image_load import * import matplotlib.pyplot as plt """ Find noise standard deviation and fit to model: noise std = a + b*sqrt(pixel mean) """ def noise(Cam, Img, plot): Cam.log += '\nProcessing image: {}'.format(Img.name) stds = [] means = [] """ iterate through macbeth square patches """ for ch_patches in Img.patches: for patch in ch_patches: """ renormalise patch """ patch = np.array(patch) patch = (patch-Img.blacklevel_16)/Img.againQ8_norm std = np.std(patch) mean = np.mean(patch) stds.append(std) means.append(mean) """ clean data and ensure all means are above 0 """ stds = np.array(stds) means = np.array(means) means = np.clip(np.array(means), 0, None) sq_means = np.sqrt(means) """ least squares fit model """ fit = np.polyfit(sq_means, stds, 1) Cam.log += '\nBlack level = {}'.format(Img.blacklevel_16) Cam.log += '\nNoise profile: offset = {}'.format(int(fit[1])) Cam.log += ' slope = {:.3f}'.format(fit[0]) """ remove any values further than std from the fit anomalies most likely caused by: > ucharacteristically noisy white patch > saturation in the white patch """ fit_score = np.abs(stds - fit[0]*sq_means - fit[1]) fit_std = np.std(stds) fit_score_norm = fit_score - fit_std anom_ind = np.where(fit_score_norm > 1) fit_score_norm.sort() sq_means_clean = np.delete(sq_means, anom_ind) stds_clean = np.delete(stds, anom_ind) removed = len(stds) - len(stds_clean) if removed != 0: Cam.log += '\nIdentified and removed {} anomalies.'.format(removed) Cam.log += '\nRecalculating fit' """ recalculate fit with outliers removed """ fit = np.polyfit(sq_means_clean, stds_clean, 1) Cam.log += '\nNoise profile: offset = {}'.format(int(fit[1])) Cam.log += ' slope = {:.3f}'.format(fit[0]) """ if fit const is < 0 then force through 0 by dividing by sq_means and fitting poly order 0 """ corrected = 0 if fit[1] < 0: corrected = 1 ones = np.ones(len(means)) y_data = stds/sq_means fit2 = np.polyfit(ones, y_data, 0) Cam.log += '\nOffset below zero. Fit recalculated with zero offset' Cam.log += '\nNoise profile: offset = 0' Cam.log += ' slope = {:.3f}'.format(fit2[0]) # print('new fit') # print(fit2) """ plot fit for debug """ if plot: x = np.arange(sq_means.max()//0.88) fit_plot = x*fit[0] + fit[1] plt.scatter(sq_means, stds, label='data', color='blue') plt.scatter(sq_means[anom_ind], stds[anom_ind], color='orange', label='anomalies') plt.plot(x, fit_plot, label='fit', color='red', ls=':') if fit[1] < 0: fit_plot_2 = x*fit2[0] plt.plot(x, fit_plot_2, label='fit 0 intercept', color='green', ls='--') plt.plot(0, 0) plt.title('Noise Plot\nImg: {}'.format(Img.str)) plt.legend(loc='upper left') plt.xlabel('Sqrt Pixel Value') plt.ylabel('Noise Standard Deviation') plt.grid() plt.show() """ End of plotting code """ """ format output to include forced 0 constant """ Cam.log += '\n' if corrected: fit = [fit2[0], 0] return fit else: return fit a> 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182