1 | """ |
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2 | TXT/IGOR 2D Q Map 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 | #See the license text in license.txt |
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9 | #copyright 2008, University of Tennessee |
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10 | ###################################################################### |
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11 | from __future__ import print_function |
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12 | |
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13 | import os |
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14 | import numpy as np |
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15 | import math |
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16 | from sas.sascalc.dataloader.data_info import Data2D, Detector |
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17 | |
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18 | # Look for unit converter |
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19 | has_converter = True |
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20 | try: |
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21 | from sas.sascalc.data_util.nxsunit import Converter |
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22 | except: |
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23 | has_converter = False |
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24 | |
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25 | |
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26 | def check_point(x_point): |
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27 | """ |
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28 | check point validity |
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29 | """ |
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30 | # set zero for non_floats |
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31 | try: |
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32 | return float(x_point) |
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33 | except: |
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34 | return 0 |
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35 | |
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36 | |
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37 | class Reader: |
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38 | """ Simple data reader for Igor data files """ |
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39 | ## File type |
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40 | type_name = "IGOR/DAT 2D Q_map" |
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41 | ## Wildcards |
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42 | type = ["IGOR/DAT 2D file in Q_map (*.dat)|*.DAT"] |
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43 | ## Extension |
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44 | ext = ['.DAT', '.dat'] |
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45 | |
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46 | def write(self, filename, data): |
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47 | """ |
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48 | Write to .dat |
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49 | |
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50 | :param filename: file name to write |
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51 | :param data: data2D |
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52 | """ |
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53 | import time |
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54 | # Write the file |
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55 | fd = open(filename, 'w') |
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56 | t = time.localtime() |
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57 | time_str = time.strftime("%H:%M on %b %d %y", t) |
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58 | |
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59 | header_str = "Data columns are Qx - Qy - I(Qx,Qy)\n\nASCII data" |
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60 | header_str += " created at %s \n\n" % time_str |
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61 | # simple 2D header |
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62 | fd.write(header_str) |
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63 | # write qx qy I values |
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64 | for i in range(len(data.data)): |
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65 | fd.write("%g %g %g\n" % (data.qx_data[i], |
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66 | data.qy_data[i], |
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67 | data.data[i])) |
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68 | # close |
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69 | fd.close() |
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70 | |
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71 | def read(self, filename=None): |
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72 | """ Read file """ |
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73 | if not os.path.isfile(filename): |
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74 | raise ValueError, \ |
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75 | "Specified file %s is not a regular file" % filename |
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76 | |
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77 | # Read file |
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78 | f = open(filename, 'r') |
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79 | buf = f.read() |
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80 | f.close() |
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81 | # Instantiate data object |
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82 | output = Data2D() |
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83 | output.filename = os.path.basename(filename) |
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84 | detector = Detector() |
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85 | if len(output.detector) > 0: |
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86 | print(str(output.detector[0])) |
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87 | output.detector.append(detector) |
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88 | |
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89 | # Get content |
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90 | dataStarted = False |
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91 | |
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92 | ## Defaults |
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93 | lines = buf.split('\n') |
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94 | x = [] |
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95 | y = [] |
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96 | |
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97 | wavelength = None |
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98 | distance = None |
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99 | transmission = None |
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100 | |
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101 | pixel_x = None |
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102 | pixel_y = None |
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103 | |
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104 | isInfo = False |
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105 | isCenter = False |
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106 | |
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107 | data_conv_q = None |
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108 | data_conv_i = None |
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109 | |
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110 | # Set units: This is the unit assumed for Q and I in the data file. |
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111 | if has_converter == True and output.Q_unit != '1/A': |
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112 | data_conv_q = Converter('1/A') |
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113 | # Test it |
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114 | data_conv_q(1.0, output.Q_unit) |
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115 | |
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116 | if has_converter == True and output.I_unit != '1/cm': |
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117 | data_conv_i = Converter('1/cm') |
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118 | # Test it |
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119 | data_conv_i(1.0, output.I_unit) |
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120 | |
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121 | |
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122 | # Remove the last lines before the for loop if the lines are empty |
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123 | # to calculate the exact number of data points |
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124 | count = 0 |
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125 | while (len(lines[len(lines) - (count + 1)].lstrip().rstrip()) < 1): |
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126 | del lines[len(lines) - (count + 1)] |
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127 | count = count + 1 |
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128 | |
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129 | #Read Header and find the dimensions of 2D data |
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130 | line_num = 0 |
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131 | # Old version NIST files: 0 |
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132 | ver = 0 |
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133 | for line in lines: |
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134 | line_num += 1 |
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135 | ## Reading the header applies only to IGOR/NIST 2D q_map data files |
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136 | # Find setup info line |
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137 | if isInfo: |
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138 | isInfo = False |
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139 | line_toks = line.split() |
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140 | # Wavelength in Angstrom |
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141 | try: |
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142 | wavelength = float(line_toks[1]) |
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143 | # Units |
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144 | if has_converter == True and \ |
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145 | output.source.wavelength_unit != 'A': |
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146 | conv = Converter('A') |
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147 | wavelength = conv(wavelength, |
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148 | units=output.source.wavelength_unit) |
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149 | except: |
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150 | #Not required |
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151 | pass |
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152 | # Distance in mm |
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153 | try: |
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154 | distance = float(line_toks[3]) |
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155 | # Units |
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156 | if has_converter == True and detector.distance_unit != 'm': |
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157 | conv = Converter('m') |
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158 | distance = conv(distance, units=detector.distance_unit) |
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159 | except: |
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160 | #Not required |
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161 | pass |
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162 | |
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163 | # Distance in meters |
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164 | try: |
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165 | transmission = float(line_toks[4]) |
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166 | except: |
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167 | #Not required |
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168 | pass |
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169 | |
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170 | if line.count("LAMBDA") > 0: |
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171 | isInfo = True |
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172 | |
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173 | # Find center info line |
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174 | if isCenter: |
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175 | isCenter = False |
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176 | line_toks = line.split() |
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177 | # Center in bin number |
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178 | center_x = float(line_toks[0]) |
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179 | center_y = float(line_toks[1]) |
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180 | |
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181 | if line.count("BCENT") > 0: |
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182 | isCenter = True |
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183 | # Check version |
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184 | if line.count("Data columns") > 0: |
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185 | if line.count("err(I)") > 0: |
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186 | ver = 1 |
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187 | # Find data start |
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188 | if line.count("ASCII data") > 0: |
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189 | dataStarted = True |
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190 | continue |
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191 | |
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192 | ## Read and get data. |
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193 | if dataStarted == True: |
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194 | line_toks = line.split() |
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195 | if len(line_toks) == 0: |
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196 | #empty line |
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197 | continue |
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198 | # the number of columns must be stayed same |
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199 | col_num = len(line_toks) |
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200 | break |
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201 | # Make numpy array to remove header lines using index |
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202 | lines_array = np.array(lines) |
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203 | |
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204 | # index for lines_array |
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205 | lines_index = np.arange(len(lines)) |
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206 | |
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207 | # get the data lines |
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208 | data_lines = lines_array[lines_index >= (line_num - 1)] |
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209 | # Now we get the total number of rows (i.e., # of data points) |
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210 | row_num = len(data_lines) |
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211 | # make it as list again to control the separators |
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212 | data_list = " ".join(data_lines.tolist()) |
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213 | # split all data to one big list w/" "separator |
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214 | data_list = data_list.split() |
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215 | |
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216 | # Check if the size is consistent with data, otherwise |
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217 | #try the tab(\t) separator |
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218 | # (this may be removed once get the confidence |
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219 | #the former working all cases). |
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220 | if len(data_list) != (len(data_lines)) * col_num: |
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221 | data_list = "\t".join(data_lines.tolist()) |
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222 | data_list = data_list.split() |
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223 | |
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224 | # Change it(string) into float |
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225 | #data_list = map(float,data_list) |
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226 | data_list1 = map(check_point, data_list) |
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227 | |
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228 | # numpy array form |
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229 | data_array = np.array(data_list1) |
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230 | # Redimesion based on the row_num and col_num, |
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231 | #otherwise raise an error. |
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232 | try: |
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233 | data_point = data_array.reshape(row_num, col_num).transpose() |
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234 | except: |
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235 | msg = "red2d_reader: Can't read this file: Not a proper file format" |
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236 | raise ValueError, msg |
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237 | ## Get the all data: Let's HARDcoding; Todo find better way |
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238 | # Defaults |
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239 | dqx_data = np.zeros(0) |
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240 | dqy_data = np.zeros(0) |
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241 | err_data = np.ones(row_num) |
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242 | qz_data = np.zeros(row_num) |
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243 | mask = np.ones(row_num, dtype=bool) |
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244 | # Get from the array |
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245 | qx_data = data_point[0] |
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246 | qy_data = data_point[1] |
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247 | data = data_point[2] |
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248 | if ver == 1: |
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249 | if col_num > (2 + ver): |
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250 | err_data = data_point[(2 + ver)] |
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251 | if col_num > (3 + ver): |
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252 | qz_data = data_point[(3 + ver)] |
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253 | if col_num > (4 + ver): |
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254 | dqx_data = data_point[(4 + ver)] |
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255 | if col_num > (5 + ver): |
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256 | dqy_data = data_point[(5 + ver)] |
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257 | #if col_num > (6 + ver): mask[data_point[(6 + ver)] < 1] = False |
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258 | q_data = np.sqrt(qx_data*qx_data+qy_data*qy_data+qz_data*qz_data) |
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259 | |
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260 | # Extra protection(it is needed for some data files): |
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261 | # If all mask elements are False, put all True |
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262 | if not mask.any(): |
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263 | mask[mask == False] = True |
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264 | |
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265 | # Store limits of the image in q space |
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266 | xmin = np.min(qx_data) |
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267 | xmax = np.max(qx_data) |
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268 | ymin = np.min(qy_data) |
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269 | ymax = np.max(qy_data) |
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270 | |
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271 | # units |
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272 | if has_converter == True and output.Q_unit != '1/A': |
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273 | xmin = data_conv_q(xmin, units=output.Q_unit) |
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274 | xmax = data_conv_q(xmax, units=output.Q_unit) |
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275 | ymin = data_conv_q(ymin, units=output.Q_unit) |
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276 | ymax = data_conv_q(ymax, units=output.Q_unit) |
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277 | |
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278 | ## calculate the range of the qx and qy_data |
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279 | x_size = math.fabs(xmax - xmin) |
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280 | y_size = math.fabs(ymax - ymin) |
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281 | |
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282 | # calculate the number of pixels in the each axes |
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283 | npix_y = math.floor(math.sqrt(len(data))) |
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284 | npix_x = math.floor(len(data) / npix_y) |
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285 | |
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286 | # calculate the size of bins |
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287 | xstep = x_size / (npix_x - 1) |
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288 | ystep = y_size / (npix_y - 1) |
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289 | |
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290 | # store x and y axis bin centers in q space |
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291 | x_bins = np.arange(xmin, xmax + xstep, xstep) |
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292 | y_bins = np.arange(ymin, ymax + ystep, ystep) |
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293 | |
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294 | # get the limits of q values |
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295 | xmin = xmin - xstep / 2 |
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296 | xmax = xmax + xstep / 2 |
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297 | ymin = ymin - ystep / 2 |
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298 | ymax = ymax + ystep / 2 |
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299 | |
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300 | #Store data in outputs |
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301 | #TODO: Check the lengths |
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302 | output.data = data |
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303 | if (err_data == 1).all(): |
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304 | output.err_data = np.sqrt(np.abs(data)) |
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305 | output.err_data[output.err_data == 0.0] = 1.0 |
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306 | else: |
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307 | output.err_data = err_data |
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308 | |
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309 | output.qx_data = qx_data |
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310 | output.qy_data = qy_data |
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311 | output.q_data = q_data |
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312 | output.mask = mask |
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313 | |
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314 | output.x_bins = x_bins |
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315 | output.y_bins = y_bins |
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316 | |
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317 | output.xmin = xmin |
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318 | output.xmax = xmax |
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319 | output.ymin = ymin |
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320 | output.ymax = ymax |
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321 | |
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322 | output.source.wavelength = wavelength |
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323 | |
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324 | # Store pixel size in mm |
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325 | detector.pixel_size.x = pixel_x |
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326 | detector.pixel_size.y = pixel_y |
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327 | |
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328 | # Store the sample to detector distance |
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329 | detector.distance = distance |
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330 | |
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331 | # optional data: if all of dq data == 0, do not pass to output |
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332 | if len(dqx_data) == len(qx_data) and dqx_data.any() != 0: |
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333 | # if no dqx_data, do not pass dqy_data. |
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334 | #(1 axis dq is not supported yet). |
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335 | if len(dqy_data) == len(qy_data) and dqy_data.any() != 0: |
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336 | # Currently we do not support dq parr, perp. |
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337 | # tranfer the comp. to cartesian coord. for newer version. |
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338 | if ver != 1: |
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339 | diag = np.sqrt(qx_data * qx_data + qy_data * qy_data) |
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340 | cos_th = qx_data / diag |
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341 | sin_th = qy_data / diag |
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342 | output.dqx_data = np.sqrt((dqx_data * cos_th) * \ |
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343 | (dqx_data * cos_th) \ |
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344 | + (dqy_data * sin_th) * \ |
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345 | (dqy_data * sin_th)) |
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346 | output.dqy_data = np.sqrt((dqx_data * sin_th) * \ |
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347 | (dqx_data * sin_th) \ |
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348 | + (dqy_data * cos_th) * \ |
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349 | (dqy_data * cos_th)) |
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350 | else: |
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351 | output.dqx_data = dqx_data |
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352 | output.dqy_data = dqy_data |
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353 | |
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354 | # Units of axes |
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355 | if data_conv_q is not None: |
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356 | output.xaxis("\\rm{Q_{x}}", output.Q_unit) |
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357 | output.yaxis("\\rm{Q_{y}}", output.Q_unit) |
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358 | else: |
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359 | output.xaxis("\\rm{Q_{x}}", 'A^{-1}') |
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360 | output.yaxis("\\rm{Q_{y}}", 'A^{-1}') |
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361 | if data_conv_i is not None: |
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362 | output.zaxis("\\rm{Intensity}", output.I_unit) |
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363 | else: |
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364 | output.zaxis("\\rm{Intensity}", "cm^{-1}") |
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365 | |
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366 | # Store loading process information |
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367 | output.meta_data['loader'] = self.type_name |
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368 | |
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369 | return output |
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