1 | """ |
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2 | Handle Q smearing |
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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 | import math |
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12 | import logging |
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13 | import sys |
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14 | |
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15 | import numpy as np # type: ignore |
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16 | from numpy import pi, exp # type:ignore |
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17 | |
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18 | from sasmodels.resolution import Slit1D, Pinhole1D |
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19 | from sasmodels.sesans import SesansTransform |
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20 | from sasmodels.resolution2d import Pinhole2D |
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21 | |
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22 | from sas.sascalc.data_util.nxsunit import Converter |
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23 | |
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24 | def smear_selection(data, model = None): |
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25 | """ |
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26 | Creates the right type of smearer according |
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27 | to the data. |
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28 | The canSAS format has a rule that either |
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29 | slit smearing data OR resolution smearing data |
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30 | is available. |
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31 | |
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32 | For the present purpose, we choose the one that |
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33 | has none-zero data. If both slit and resolution |
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34 | smearing arrays are filled with good data |
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35 | (which should not happen), then we choose the |
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36 | resolution smearing data. |
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37 | |
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38 | :param data: Data1D object |
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39 | :param model: sas.model instance |
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40 | """ |
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41 | # Sanity check. If we are not dealing with a SAS Data1D |
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42 | # object, just return None |
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43 | # This checks for 2D data (does not throw exception because fail is common) |
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44 | if data.__class__.__name__ not in ['Data1D', 'Theory1D']: |
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45 | if data is None: |
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46 | return None |
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47 | elif data.dqx_data is None or data.dqy_data is None: |
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48 | return None |
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49 | return PySmear2D(data) |
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50 | # This checks for 1D data with smearing info in the data itself (again, fail is likely; no exceptions) |
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51 | if not hasattr(data, "dx") and not hasattr(data, "dxl")\ |
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52 | and not hasattr(data, "dxw"): |
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53 | return None |
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54 | |
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55 | # Look for resolution smearing data |
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56 | # This is the code that checks for SESANS data; it looks for the file loader |
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57 | # TODO: change other sanity checks to check for file loader instead of data structure? |
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58 | _found_sesans = False |
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59 | #if data.dx is not None and data.meta_data['loader']=='SESANS': |
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60 | if data.dx is not None and data.isSesans: |
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61 | #if data.dx[0] > 0.0: |
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62 | if np.size(data.dx[data.dx <= 0]) == 0: |
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63 | _found_sesans = True |
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64 | # if data.dx[0] <= 0.0: |
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65 | if np.size(data.dx[data.dx <= 0]) > 0: |
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66 | raise ValueError('one or more of your dx values are negative, please check the data file!') |
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67 | |
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68 | if _found_sesans: |
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69 | # Pre-compute the Hankel matrix (H) |
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70 | SElength = Converter(data._xunit)(data.x, "A") |
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71 | |
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72 | theta_max = Converter("radians")(data.sample.zacceptance)[0] |
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73 | q_max = 2 * np.pi / np.max(data.source.wavelength) * np.sin(theta_max) |
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74 | zaccept = Converter("1/A")(q_max, "1/" + data.source.wavelength_unit), |
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75 | |
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76 | Rmax = 10000000 |
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77 | hankel = SesansTransform(data.x, SElength, |
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78 | data.source.wavelength, |
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79 | zaccept, Rmax) |
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80 | # Then return the actual transform, as if it were a smearing function |
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81 | return PySmear(hankel, model, offset=0) |
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82 | |
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83 | _found_resolution = False |
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84 | if data.dx is not None and len(data.dx) == len(data.x): |
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85 | |
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86 | # Check that we have non-zero data |
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87 | if data.dx[0] > 0.0: |
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88 | _found_resolution = True |
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89 | #print "_found_resolution",_found_resolution |
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90 | #print "data1D.dx[0]",data1D.dx[0],data1D.dxl[0] |
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91 | # If we found resolution smearing data, return a QSmearer |
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92 | if _found_resolution == True: |
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93 | return pinhole_smear(data, model) |
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94 | |
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95 | # Look for slit smearing data |
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96 | _found_slit = False |
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97 | if data.dxl is not None and len(data.dxl) == len(data.x) \ |
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98 | and data.dxw is not None and len(data.dxw) == len(data.x): |
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99 | |
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100 | # Check that we have non-zero data |
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101 | if data.dxl[0] > 0.0 or data.dxw[0] > 0.0: |
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102 | _found_slit = True |
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103 | |
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104 | # Sanity check: all data should be the same as a function of Q |
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105 | for item in data.dxl: |
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106 | if data.dxl[0] != item: |
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107 | _found_resolution = False |
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108 | break |
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109 | |
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110 | for item in data.dxw: |
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111 | if data.dxw[0] != item: |
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112 | _found_resolution = False |
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113 | break |
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114 | # If we found slit smearing data, return a slit smearer |
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115 | if _found_slit == True: |
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116 | return slit_smear(data, model) |
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117 | return None |
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118 | |
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119 | |
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120 | class PySmear(object): |
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121 | """ |
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122 | Wrapper for pure python sasmodels resolution functions. |
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123 | """ |
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124 | def __init__(self, resolution, model, offset=None): |
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125 | self.model = model |
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126 | self.resolution = resolution |
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127 | if offset is None: |
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128 | offset = np.searchsorted(self.resolution.q_calc, self.resolution.q[0]) |
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129 | self.offset = offset |
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130 | |
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131 | def apply(self, iq_in, first_bin=0, last_bin=None): |
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132 | """ |
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133 | Apply the resolution function to the data. |
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134 | Note that this is called with iq_in matching data.x, but with |
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135 | iq_in[first_bin:last_bin] set to theory values for these bins, |
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136 | and the remainder left undefined. The first_bin, last_bin values |
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137 | should be those returned from get_bin_range. |
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138 | The returned value is of the same length as iq_in, with the range |
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139 | first_bin:last_bin set to the resolution smeared values. |
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140 | """ |
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141 | if last_bin is None: last_bin = len(iq_in) |
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142 | start, end = first_bin + self.offset, last_bin + self.offset |
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143 | q_calc = self.resolution.q_calc |
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144 | iq_calc = np.empty_like(q_calc) |
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145 | if start > 0: |
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146 | iq_calc[:start] = self.model.evalDistribution(q_calc[:start]) |
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147 | if end+1 < len(q_calc): |
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148 | iq_calc[end+1:] = self.model.evalDistribution(q_calc[end+1:]) |
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149 | iq_calc[start:end+1] = iq_in[first_bin:last_bin+1] |
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150 | smeared = self.resolution.apply(iq_calc) |
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151 | return smeared |
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152 | __call__ = apply |
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153 | |
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154 | def get_bin_range(self, q_min=None, q_max=None): |
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155 | """ |
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156 | For a given q_min, q_max, find the corresponding indices in the data. |
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157 | Returns first, last. |
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158 | Note that these are indexes into q from the data, not the q_calc |
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159 | needed by the resolution function. Note also that these are the |
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160 | indices, not the range limits. That is, the complete range will be |
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161 | q[first:last+1]. |
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162 | """ |
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163 | q = self.resolution.q |
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164 | first = np.searchsorted(q, q_min) |
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165 | last = np.searchsorted(q, q_max) |
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166 | return first, min(last,len(q)-1) |
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167 | |
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168 | def slit_smear(data, model=None): |
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169 | q = data.x |
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170 | width = data.dxw if data.dxw is not None else 0 |
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171 | height = data.dxl if data.dxl is not None else 0 |
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172 | # TODO: width and height seem to be reversed |
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173 | return PySmear(Slit1D(q, height, width), model) |
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174 | |
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175 | def pinhole_smear(data, model=None): |
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176 | q = data.x |
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177 | width = data.dx if data.dx is not None else 0 |
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178 | return PySmear(Pinhole1D(q, width), model) |
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179 | |
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180 | |
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181 | class PySmear2D(object): |
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182 | """ |
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183 | Q smearing class for SAS 2d pinhole data |
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184 | """ |
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185 | |
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186 | def __init__(self, data=None, model=None): |
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187 | self.data = data |
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188 | self.model = model |
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189 | self.accuracy = 'Low' |
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190 | self.limit = 3.0 |
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191 | self.index = None |
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192 | self.coords = 'polar' |
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193 | self.smearer = True |
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194 | |
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195 | def set_accuracy(self, accuracy='Low'): |
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196 | """ |
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197 | Set accuracy. |
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198 | |
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199 | :param accuracy: string |
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200 | """ |
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201 | self.accuracy = accuracy |
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202 | |
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203 | def set_smearer(self, smearer=True): |
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204 | """ |
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205 | Set whether or not smearer will be used |
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206 | |
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207 | :param smearer: smear object |
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208 | |
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209 | """ |
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210 | self.smearer = smearer |
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211 | |
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212 | def set_data(self, data=None): |
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213 | """ |
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214 | Set data. |
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215 | |
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216 | :param data: DataLoader.Data_info type |
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217 | """ |
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218 | self.data = data |
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219 | |
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220 | def set_model(self, model=None): |
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221 | """ |
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222 | Set model. |
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223 | |
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224 | :param model: sas.models instance |
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225 | """ |
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226 | self.model = model |
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227 | |
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228 | def set_index(self, index=None): |
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229 | """ |
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230 | Set index. |
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231 | |
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232 | :param index: 1d arrays |
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233 | """ |
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234 | self.index = index |
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235 | |
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236 | def get_value(self): |
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237 | """ |
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238 | Over sampling of r_nbins times phi_nbins, calculate Gaussian weights, |
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239 | then find smeared intensity |
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240 | """ |
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241 | if self.smearer: |
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242 | res = Pinhole2D(data=self.data, index=self.index, |
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243 | nsigma=3.0, accuracy=self.accuracy, |
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244 | coords=self.coords) |
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245 | val = self.model.evalDistribution(res.q_calc) |
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246 | return res.apply(val) |
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247 | else: |
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248 | index = self.index if self.index is not None else slice(None) |
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249 | qx_data = self.data.qx_data[index] |
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250 | qy_data = self.data.qy_data[index] |
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251 | q_calc = [qx_data, qy_data] |
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252 | val = self.model.evalDistribution(q_calc) |
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253 | return val |
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254 | |
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