1 | """ |
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2 | IGOR 2D reduced file reader |
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3 | """ |
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4 | ############################################################################ |
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5 | #This software was developed by the University of Tennessee as part of the |
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6 | #Distributed Data Analysis of Neutron Scattering Experiments (DANSE) |
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7 | #project funded by the US National Science Foundation. |
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8 | #If you use DANSE applications to do scientific research that leads to |
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9 | #publication, we ask that you acknowledge the use of the software with the |
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10 | #following sentence: |
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11 | #This work benefited from DANSE software developed under NSF award DMR-0520547. |
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12 | #copyright 2008, University of Tennessee |
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13 | ############################################################################# |
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14 | import os |
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15 | |
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16 | from sas.sascalc.dataloader.data_info import Data2D |
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17 | from sas.sascalc.dataloader.data_info import Detector |
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18 | from sas.sascalc.dataloader.manipulations import reader2D_converter |
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19 | import numpy as np |
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20 | |
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21 | # Look for unit converter |
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22 | has_converter = True |
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23 | try: |
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24 | from sas.sascalc.data_util.nxsunit import Converter |
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25 | except: |
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26 | has_converter = False |
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27 | |
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28 | |
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29 | class Reader: |
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30 | """ Simple data reader for Igor data files """ |
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31 | ## File type |
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32 | type_name = "IGOR 2D" |
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33 | ## Wildcards |
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34 | type = ["IGOR 2D files (*.ASC)|*.ASC"] |
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35 | ## Extension |
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36 | ext=['.ASC', '.asc'] |
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37 | |
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38 | def read(self, filename=None): |
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39 | """ Read file """ |
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40 | if not os.path.isfile(filename): |
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41 | raise ValueError("Specified file %s is not a regular " |
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42 | "file" % filename) |
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43 | |
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44 | output = Data2D() |
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45 | |
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46 | output.filename = os.path.basename(filename) |
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47 | detector = Detector() |
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48 | if len(output.detector): |
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49 | print(str(output.detector[0])) |
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50 | output.detector.append(detector) |
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51 | |
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52 | data_conv_q = data_conv_i = None |
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53 | |
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54 | if has_converter and output.Q_unit != '1/A': |
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55 | data_conv_q = Converter('1/A') |
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56 | # Test it |
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57 | data_conv_q(1.0, output.Q_unit) |
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58 | |
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59 | if has_converter and output.I_unit != '1/cm': |
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60 | data_conv_i = Converter('1/cm') |
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61 | # Test it |
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62 | data_conv_i(1.0, output.I_unit) |
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63 | |
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64 | data_row = 0 |
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65 | wavelength = distance = center_x = center_y = None |
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66 | dataStarted = isInfo = isCenter = False |
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67 | |
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68 | with open(filename, 'r') as f: |
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69 | for line in f: |
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70 | data_row += 1 |
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71 | # Find setup info line |
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72 | if isInfo: |
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73 | isInfo = False |
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74 | line_toks = line.split() |
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75 | # Wavelength in Angstrom |
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76 | try: |
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77 | wavelength = float(line_toks[1]) |
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78 | except ValueError: |
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79 | msg = "IgorReader: can't read this file, missing wavelength" |
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80 | raise ValueError(msg) |
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81 | # Distance in meters |
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82 | try: |
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83 | distance = float(line_toks[3]) |
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84 | except ValueError: |
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85 | msg = "IgorReader: can't read this file, missing distance" |
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86 | raise ValueError(msg) |
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87 | |
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88 | # Distance in meters |
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89 | try: |
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90 | transmission = float(line_toks[4]) |
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91 | except: |
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92 | msg = "IgorReader: can't read this file, " |
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93 | msg += "missing transmission" |
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94 | raise ValueError(msg) |
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95 | |
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96 | if line.count("LAMBDA"): |
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97 | isInfo = True |
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98 | |
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99 | # Find center info line |
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100 | if isCenter: |
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101 | isCenter = False |
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102 | line_toks = line.split() |
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103 | |
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104 | # Center in bin number: Must subtract 1 because |
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105 | # the index starts from 1 |
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106 | center_x = float(line_toks[0]) - 1 |
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107 | center_y = float(line_toks[1]) - 1 |
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108 | |
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109 | if line.count("BCENT"): |
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110 | isCenter = True |
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111 | |
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112 | # Find data start |
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113 | if line.count("***"): |
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114 | # now have to continue to blank line |
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115 | dataStarted = True |
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116 | |
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117 | # Check that we have all the info |
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118 | if (wavelength is None |
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119 | or distance is None |
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120 | or center_x is None |
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121 | or center_y is None): |
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122 | msg = "IgorReader:Missing information in data file" |
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123 | raise ValueError(msg) |
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124 | |
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125 | if dataStarted: |
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126 | if len(line.rstrip()): |
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127 | continue |
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128 | else: |
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129 | break |
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130 | |
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131 | # The data is loaded in row major order (last index changing most |
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132 | # rapidly). However, the original data is in column major order (first |
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133 | # index changing most rapidly). The swap to column major order is done |
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134 | # in reader2D_converter at the end of this method. |
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135 | data = np.loadtxt(filename, skiprows=data_row) |
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136 | size_x = size_y = int(np.rint(np.sqrt(data.size))) |
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137 | output.data = np.reshape(data, (size_x, size_y)) |
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138 | output.err_data = np.zeros_like(output.data) |
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139 | |
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140 | # Det 640 x 640 mm |
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141 | # Q = 4 * pi/lambda * sin(theta/2) |
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142 | # Bin size is 0.5 cm |
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143 | # Removed +1 from theta = (i_x - center_x + 1)*0.5 / distance |
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144 | # / 100.0 and |
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145 | # Removed +1 from theta = (i_y - center_y + 1)*0.5 / |
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146 | # distance / 100.0 |
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147 | # ToDo: Need complete check if the following |
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148 | # convert process is consistent with fitting.py. |
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149 | |
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150 | # calculate qx, qy bin centers of each pixel in the image |
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151 | theta = (np.arange(size_x) - center_x) * 0.5 / distance / 100. |
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152 | qx = 4 * np.pi / wavelength * np.sin(theta/2) |
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153 | |
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154 | theta = (np.arange(size_y) - center_y) * 0.5 / distance / 100. |
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155 | qy = 4 * np.pi / wavelength * np.sin(theta/2) |
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156 | |
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157 | if has_converter and output.Q_unit != '1/A': |
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158 | qx = data_conv_q(qx, units=output.Q_unit) |
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159 | qy = data_conv_q(qx, units=output.Q_unit) |
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160 | |
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161 | xmax = np.max(qx) |
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162 | xmin = np.min(qx) |
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163 | ymax = np.max(qy) |
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164 | ymin = np.min(qy) |
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165 | |
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166 | # calculate edge offset in q. |
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167 | theta = 0.25 / distance / 100.0 |
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168 | xstep = 4.0 * np.pi / wavelength * np.sin(theta / 2.0) |
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169 | |
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170 | theta = 0.25 / distance / 100.0 |
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171 | ystep = 4.0 * np.pi/ wavelength * np.sin(theta / 2.0) |
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172 | |
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173 | # Store all data ###################################### |
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174 | # Store wavelength |
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175 | if has_converter and output.source.wavelength_unit != 'A': |
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176 | conv = Converter('A') |
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177 | wavelength = conv(wavelength, units=output.source.wavelength_unit) |
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178 | output.source.wavelength = wavelength |
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179 | |
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180 | # Store distance |
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181 | if has_converter and detector.distance_unit != 'm': |
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182 | conv = Converter('m') |
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183 | distance = conv(distance, units=detector.distance_unit) |
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184 | detector.distance = distance |
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185 | |
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186 | # Store transmission |
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187 | output.sample.transmission = transmission |
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188 | |
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189 | # Store pixel size (mm) |
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190 | pixel = 5.0 |
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191 | if has_converter and detector.pixel_size_unit != 'mm': |
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192 | conv = Converter('mm') |
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193 | pixel = conv(pixel, units=detector.pixel_size_unit) |
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194 | detector.pixel_size.x = pixel |
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195 | detector.pixel_size.y = pixel |
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196 | |
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197 | # Store beam center in distance units |
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198 | detector.beam_center.x = center_x * pixel |
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199 | detector.beam_center.y = center_y * pixel |
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200 | |
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201 | # Store limits of the image (2D array) |
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202 | xmin -= xstep / 2.0 |
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203 | xmax += xstep / 2.0 |
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204 | ymin -= ystep / 2.0 |
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205 | ymax += ystep / 2.0 |
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206 | if has_converter and output.Q_unit != '1/A': |
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207 | xmin = data_conv_q(xmin, units=output.Q_unit) |
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208 | xmax = data_conv_q(xmax, units=output.Q_unit) |
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209 | ymin = data_conv_q(ymin, units=output.Q_unit) |
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210 | ymax = data_conv_q(ymax, units=output.Q_unit) |
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211 | output.xmin = xmin |
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212 | output.xmax = xmax |
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213 | output.ymin = ymin |
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214 | output.ymax = ymax |
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215 | |
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216 | # Store x and y axis bin centers |
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217 | output.x_bins = qx.tolist() |
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218 | output.y_bins = qy.tolist() |
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219 | |
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220 | # Units |
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221 | if data_conv_q is not None: |
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222 | output.xaxis("\\rm{Q_{x}}", output.Q_unit) |
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223 | output.yaxis("\\rm{Q_{y}}", output.Q_unit) |
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224 | else: |
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225 | output.xaxis("\\rm{Q_{x}}", 'A^{-1}') |
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226 | output.yaxis("\\rm{Q_{y}}", 'A^{-1}') |
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227 | |
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228 | if data_conv_i is not None: |
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229 | output.zaxis("\\rm{Intensity}", output.I_unit) |
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230 | else: |
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231 | output.zaxis("\\rm{Intensity}", "cm^{-1}") |
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232 | |
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233 | # Store loading process information |
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234 | output.meta_data['loader'] = self.type_name |
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235 | output = reader2D_converter(output) |
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236 | |
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237 | return output |
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