1 | # File: ReduceOneSCD_Run.py |
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2 | # |
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3 | # Version 2.0, modified to work with Mantid's new python interface. |
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4 | # |
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5 | # This script will reduce one SCD run. The configuration file name and |
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6 | # the run to be processed must be specified as the first two command line |
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7 | # parameters. This script is intended to be run in parallel using the |
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8 | # ReduceSCD_Parallel.py script, after this script and configuration file has |
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9 | # been tested to work properly for one run. This script will load, find peaks, |
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10 | # index and integrate either found or predicted peaks for the specified run. |
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11 | # Either sphere integration or the Mantid PeakIntegration algorithms are |
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12 | # currently supported, but it may be updated to support other integration |
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13 | # methods. Users should make a directory to hold the output of this script, |
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14 | # and must specify that output directory in the configuration file that |
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15 | # provides the parameters to this script. |
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16 | # |
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17 | # NOTE: All of the parameters that the user must specify are listed with |
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18 | # instructive comments in the sample configuration file: ReduceSCD.config. |
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19 | # |
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20 | |
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21 | # |
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22 | # _v1: December 3rd 2013. Mads Joergensen |
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23 | # This version now includes the posibility to use the 1D cylindrical integration method |
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24 | # and the posibility to load a UB matrix which will be used for integration of the individual |
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25 | # runs and to index the combined file (Code from Xiapoing). |
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26 | # |
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27 | |
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28 | |
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29 | import os |
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30 | import sys |
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31 | import shutil |
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32 | import time |
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33 | import ReduceDictionary |
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34 | #sys.path.append("/opt/mantidnightly/bin") |
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35 | sys.path.append("/opt/Mantid/bin") |
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36 | |
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37 | from mantid.simpleapi import * |
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38 | from mantid.api import * |
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39 | |
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40 | print "API Version" |
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41 | print apiVersion() |
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42 | |
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43 | start_time = time.time() |
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44 | |
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45 | # |
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46 | # Get the config file name and the run number to process from the command line |
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47 | # |
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48 | if (len(sys.argv) < 3): |
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49 | print "You MUST give the config file name and run number on the command line" |
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50 | exit(0) |
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51 | |
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52 | config_file_name = sys.argv[1] |
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53 | run = sys.argv[2] |
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54 | |
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55 | # |
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56 | # Load the parameter names and values from the specified configuration file |
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57 | # into a dictionary and set all the required parameters from the dictionary. |
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58 | # |
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59 | params_dictionary = ReduceDictionary.LoadDictionary( config_file_name ) |
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60 | |
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61 | instrument_name = params_dictionary[ "instrument_name" ] |
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62 | calibration_file_1 = params_dictionary[ "calibration_file_1" ] |
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63 | calibration_file_2 = params_dictionary[ "calibration_file_2" ] |
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64 | data_directory = params_dictionary[ "data_directory" ] |
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65 | output_directory = params_dictionary[ "output_directory" ] |
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66 | min_tof = params_dictionary[ "min_tof" ] |
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67 | max_tof = params_dictionary[ "max_tof" ] |
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68 | min_monitor_tof = params_dictionary[ "min_monitor_tof" ] |
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69 | max_monitor_tof = params_dictionary[ "max_monitor_tof" ] |
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70 | monitor_index = params_dictionary[ "monitor_index" ] |
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71 | cell_type = params_dictionary[ "cell_type" ] |
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72 | centering = params_dictionary[ "centering" ] |
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73 | num_peaks_to_find = params_dictionary[ "num_peaks_to_find" ] |
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74 | min_d = params_dictionary[ "min_d" ] |
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75 | max_d = params_dictionary[ "max_d" ] |
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76 | tolerance = params_dictionary[ "tolerance" ] |
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77 | integrate_predicted_peaks = params_dictionary[ "integrate_predicted_peaks" ] |
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78 | min_pred_wl = params_dictionary[ "min_pred_wl" ] |
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79 | max_pred_wl = params_dictionary[ "max_pred_wl" ] |
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80 | min_pred_dspacing = params_dictionary[ "min_pred_dspacing" ] |
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81 | max_pred_dspacing = params_dictionary[ "max_pred_dspacing" ] |
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82 | |
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83 | use_sphere_integration = params_dictionary[ "use_sphere_integration" ] |
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84 | use_ellipse_integration = params_dictionary[ "use_ellipse_integration" ] |
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85 | use_fit_peaks_integration = params_dictionary[ "use_fit_peaks_integration" ] |
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86 | use_cylindrical_integration = params_dictionary[ "use_cylindrical_integration" ] |
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87 | |
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88 | peak_radius = params_dictionary[ "peak_radius" ] |
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89 | bkg_inner_radius = params_dictionary[ "bkg_inner_radius" ] |
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90 | bkg_outer_radius = params_dictionary[ "bkg_outer_radius" ] |
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91 | integrate_if_edge_peak = params_dictionary[ "integrate_if_edge_peak" ] |
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92 | |
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93 | rebin_step = params_dictionary[ "rebin_step" ] |
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94 | preserve_events = params_dictionary[ "preserve_events" ] |
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95 | use_ikeda_carpenter = params_dictionary[ "use_ikeda_carpenter" ] |
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96 | n_bad_edge_pixels = params_dictionary[ "n_bad_edge_pixels" ] |
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97 | |
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98 | rebin_params = min_tof + "," + rebin_step + "," + max_tof |
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99 | |
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100 | ellipse_region_radius = params_dictionary[ "ellipse_region_radius" ] |
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101 | ellipse_size_specified = params_dictionary[ "ellipse_size_specified" ] |
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102 | |
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103 | cylinder_radius = params_dictionary[ "cylinder_radius" ] |
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104 | cylinder_length = params_dictionary[ "cylinder_length" ] |
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105 | |
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106 | read_UB = params_dictionary[ "read_UB" ] |
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107 | UB_filename = params_dictionary[ "UB_filename" ] |
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108 | |
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109 | # |
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110 | # Get the fully qualified input run file name, either from a specified data |
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111 | # directory or from findnexus |
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112 | # |
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113 | if data_directory is not None: |
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114 | full_name = data_directory + "/" + instrument_name + "_" + run + "_event.nxs" |
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115 | else: |
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116 | temp_buffer = os.popen("findnexus --event -i "+instrument_name+" "+str(run) ) |
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117 | full_name = temp_buffer.readline() |
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118 | full_name=full_name.strip() |
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119 | if not full_name.endswith('nxs'): |
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120 | print "Exiting since the data_directory was not specified and" |
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121 | print "findnexus failed for event NeXus file: " + instrument_name + " " + str(run) |
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122 | exit(0) |
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123 | |
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124 | print "\nProcessing File: " + full_name + " ......\n" |
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125 | |
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126 | # |
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127 | # Name the files to write for this run |
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128 | # |
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129 | run_niggli_matrix_file = output_directory + "/" + run + "_Niggli.mat" |
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130 | run_niggli_integrate_file = output_directory + "/" + run + "_Niggli.integrate" |
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131 | |
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132 | # |
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133 | # Load the run data and find the total monitor counts |
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134 | # |
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135 | event_ws = LoadEventNexus( Filename=full_name, |
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136 | FilterByTofMin=min_tof, FilterByTofMax=max_tof ) |
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137 | |
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138 | # |
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139 | # Load calibration file(s) if specified. NOTE: The file name passed in to LoadIsawDetCal |
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140 | # can not be None. TOPAZ has one calibration file, but SNAP may have two. |
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141 | # |
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142 | if (calibration_file_1 is not None ) or (calibration_file_2 is not None): |
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143 | if (calibration_file_1 is None ): |
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144 | calibration_file_1 = "" |
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145 | if (calibration_file_2 is None ): |
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146 | calibration_file_2 = "" |
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147 | LoadIsawDetCal( event_ws, |
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148 | Filename=calibration_file_1, Filename2=calibration_file_2 ) |
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149 | |
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150 | monitor_ws = LoadNexusMonitors( Filename=full_name ) |
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151 | |
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152 | integrated_monitor_ws = Integration( InputWorkspace=monitor_ws, |
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153 | RangeLower=min_monitor_tof, RangeUpper=max_monitor_tof, |
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154 | StartWorkspaceIndex=monitor_index, EndWorkspaceIndex=monitor_index ) |
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155 | |
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156 | monitor_count = integrated_monitor_ws.dataY(0)[0] |
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157 | print "\n", run, " has calculated monitor count", monitor_count, "\n" |
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158 | |
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159 | # |
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160 | # Make MD workspace using Lorentz correction, to find peaks |
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161 | # |
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162 | MDEW = ConvertToMD( InputWorkspace=event_ws, QDimensions="Q3D", |
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163 | dEAnalysisMode="Elastic", QConversionScales="Q in A^-1", |
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164 | LorentzCorrection='1', MinValues="-50,-50,-50", MaxValues="50,50,50", |
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165 | SplitInto='2', SplitThreshold='50',MaxRecursionDepth='11' ) |
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166 | # |
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167 | # Find the requested number of peaks. Once the peaks are found, we no longer |
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168 | # need the weighted MD event workspace, so delete it. |
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169 | # |
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170 | distance_threshold = 0.9 * 6.28 / float(max_d) |
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171 | peaks_ws = FindPeaksMD( MDEW, MaxPeaks=num_peaks_to_find, |
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172 | PeakDistanceThreshold=distance_threshold ) |
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173 | AnalysisDataService.remove( MDEW.getName() ) |
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174 | |
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175 | # Read or find UB for the run |
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176 | if read_UB: |
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177 | # Read orientation matrix from file |
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178 | LoadIsawUB(InputWorkspace=peaks_ws, Filename=UB_filename) |
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179 | else: |
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180 | # Find a Niggli UB matrix that indexes the peaks in this run |
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181 | FindUBUsingFFT( PeaksWorkspace=peaks_ws, MinD=min_d, MaxD=max_d, Tolerance=tolerance ) |
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182 | |
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183 | IndexPeaks( PeaksWorkspace=peaks_ws, Tolerance=tolerance) |
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184 | |
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185 | |
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186 | # |
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187 | # Save UB and peaks file, so if something goes wrong latter, we can at least |
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188 | # see these partial results |
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189 | # |
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190 | SaveIsawUB( InputWorkspace=peaks_ws,Filename=run_niggli_matrix_file ) |
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191 | SaveIsawPeaks( InputWorkspace=peaks_ws, AppendFile=False, |
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192 | Filename=run_niggli_integrate_file ) |
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193 | |
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194 | # |
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195 | # Get complete list of peaks to be integrated and load the UB matrix into |
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196 | # the predicted peaks workspace, so that information can be used by the |
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197 | # PeakIntegration algorithm. |
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198 | # |
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199 | if integrate_predicted_peaks: |
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200 | print "PREDICTING peaks to integrate...." |
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201 | peaks_ws = PredictPeaks( InputWorkspace=peaks_ws, |
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202 | WavelengthMin=min_pred_wl, WavelengthMax=max_pred_wl, |
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203 | MinDSpacing=min_pred_dspacing, MaxDSpacing=max_pred_dspacing, |
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204 | ReflectionCondition='Primitive' ) |
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205 | else: |
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206 | print "Only integrating FOUND peaks ...." |
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207 | # |
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208 | # Set the monitor counts for all the peaks that will be integrated |
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209 | # |
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210 | num_peaks = peaks_ws.getNumberPeaks() |
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211 | for i in range(num_peaks): |
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212 | peak = peaks_ws.getPeak(i) |
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213 | peak.setMonitorCount( monitor_count ) |
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214 | |
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215 | if use_sphere_integration: |
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216 | # |
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217 | # Integrate found or predicted peaks in Q space using spheres, and save |
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218 | # integrated intensities, with Niggli indexing. First get an un-weighted |
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219 | # workspace to do raw integration (we don't need high resolution or |
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220 | # LorentzCorrection to do the raw sphere integration ) |
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221 | # |
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222 | MDEW = ConvertToMD( InputWorkspace=event_ws, QDimensions="Q3D", |
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223 | dEAnalysisMode="Elastic", QConversionScales="Q in A^-1", |
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224 | LorentzCorrection='0', MinValues="-50,-50,-50", MaxValues="50,50,50", |
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225 | SplitInto='2', SplitThreshold='500',MaxRecursionDepth='10' ) |
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226 | |
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227 | peaks_ws = IntegratePeaksMD( InputWorkspace=MDEW, PeakRadius=peak_radius, |
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228 | CoordinatesToUse="Q (sample frame)", |
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229 | BackgroundOuterRadius=bkg_outer_radius, |
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230 | BackgroundInnerRadius=bkg_inner_radius, |
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231 | PeaksWorkspace=peaks_ws, |
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232 | IntegrateIfOnEdge=integrate_if_edge_peak ) |
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233 | |
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234 | elif use_fit_peaks_integration: |
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235 | event_ws = Rebin( InputWorkspace=event_ws, |
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236 | Params=rebin_params, PreserveEvents=preserve_events ) |
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237 | peaks_ws = PeakIntegration( InPeaksWorkspace=peaks_ws, InputWorkspace=event_ws, |
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238 | IkedaCarpenterTOF=use_ikeda_carpenter, |
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239 | MatchingRunNo=True, |
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240 | NBadEdgePixels=n_bad_edge_pixels ) |
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241 | |
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242 | elif use_ellipse_integration: |
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243 | peaks_ws= IntegrateEllipsoids( InputWorkspace=event_ws, PeaksWorkspace = peaks_ws, |
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244 | RegionRadius = ellipse_region_radius, |
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245 | SpecifySize = ellipse_size_specified, |
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246 | PeakSize = peak_radius, |
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247 | BackgroundOuterSize = bkg_outer_radius, |
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248 | BackgroundInnerSize = bkg_inner_radius ) |
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249 | |
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250 | elif use_cylindrical_integration: |
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251 | profiles_filename = output_directory + "/" + instrument_name + '_' + run + '.profiles' |
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252 | MDEW = ConvertToMD( InputWorkspace=event_ws, QDimensions="Q3D", |
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253 | dEAnalysisMode="Elastic", QConversionScales="Q in A^-1", |
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254 | LorentzCorrection='0', MinValues="-50,-50,-50", MaxValues="50,50,50", |
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255 | SplitInto='2', SplitThreshold='500',MaxRecursionDepth='10' ) |
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256 | |
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257 | peaks_ws = IntegratePeaksMD( InputWorkspace=MDEW, PeakRadius=cylinder_radius, |
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258 | CoordinatesToUse="Q (sample frame)", |
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259 | Cylinder='1', CylinderLength = cylinder_length, |
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260 | PercentBackground = '20', ProfileFunction = 'NoFit', |
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261 | ProfilesFile = profiles_filename, |
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262 | PeaksWorkspace=peaks_ws, |
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263 | ) |
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264 | if (not cell_type is None) and (not centering is None): |
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265 | print "WARNING: Cylindrical profiles are NOT transformed!!!" |
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266 | |
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267 | # |
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268 | # Save the final integrated peaks, using the Niggli reduced cell. |
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269 | # This is the only file needed, for the driving script to get a combined |
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270 | # result. |
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271 | # |
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272 | SaveIsawPeaks( InputWorkspace=peaks_ws, AppendFile=False, |
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273 | Filename=run_niggli_integrate_file ) |
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274 | |
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275 | # Print warning if user is trying to integrate using the cylindrical method and transorm the cell |
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276 | if use_cylindrical_integration: |
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277 | if (not cell_type is None) or (not centering is None): |
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278 | print "WARNING: Cylindrical profiles are NOT transformed!!!" |
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279 | # |
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280 | # If requested, also switch to the specified conventional cell and save the |
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281 | # corresponding matrix and integrate file |
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282 | # |
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283 | if not use_ellipse_integration: |
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284 | if (not cell_type is None) and (not centering is None) : |
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285 | run_conventional_matrix_file = output_directory + "/" + run + "_" + \ |
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286 | cell_type + "_" + centering + ".mat" |
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287 | run_conventional_integrate_file = output_directory + "/" + run + "_" + \ |
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288 | cell_type + "_" + centering + ".integrate" |
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289 | SelectCellOfType( PeaksWorkspace=peaks_ws, |
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290 | CellType=cell_type, Centering=centering, |
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291 | Apply=True, Tolerance=tolerance ) |
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292 | SaveIsawPeaks( InputWorkspace=peaks_ws, AppendFile=False, |
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293 | Filename=run_conventional_integrate_file ) |
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294 | SaveIsawUB( InputWorkspace=peaks_ws, Filename=run_conventional_matrix_file ) |
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295 | |
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296 | end_time = time.time() |
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297 | print '\nReduced run ' + str(run) + ' in ' + str(end_time - start_time) + ' sec' |
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298 | print 'using config file ' + config_file_name |
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299 | |
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300 | # |
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301 | # Try to get this to terminate when run by ReduceSCD_Parallel.py, from NX session |
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302 | # |
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303 | sys.exit(0) |
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304 | |
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