1 | /* ======================================================================== *\
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2 | !
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3 | ! *
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4 | ! * This file is part of MARS, the MAGIC Analysis and Reconstruction
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5 | ! * Software. It is distributed to you in the hope that it can be a useful
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6 | ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes.
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7 | ! * It is distributed WITHOUT ANY WARRANTY.
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8 | ! *
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9 | ! * Permission to use, copy, modify and distribute this software and its
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10 | ! * documentation for any purpose is hereby granted without fee,
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11 | ! * provided that the above copyright notice appear in all copies and
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12 | ! * that both that copyright notice and this permission notice appear
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13 | ! * in supporting documentation. It is provided "as is" without express
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14 | ! * or implied warranty.
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15 | ! *
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16 | !
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17 | !
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18 | ! Author(s): Marcos Lopez 10/2003 <mailto:marcos@gae.ucm.es>
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19 | !
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20 | ! Copyright: MAGIC Software Development, 2000-2003
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21 | !
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22 | !
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23 | \* ======================================================================== */
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24 |
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25 | //////////////////////////////////////////////////////////////////////////////
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26 | //
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27 | // MMcWeightEnergySlopeCalc
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28 | //
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29 | // Change the spectrum of the MC showers simulated with Corsika (a power law)
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30 | // to a new one, which can be either, again a power law but with a different
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31 | // spectral index, or a generalizeed spectrum. The new spectrum can be
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32 | // pass to this class in different ways:
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33 | // 1. Is the new spectrum will be a power law, just introduce the slope
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34 | // of this power law.
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35 | // 2. Is the new spectrum will have a general shape, different options are
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36 | // available:
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37 | // a) The new spectrum is pass as a TF1 function
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38 | // b) The new spectrum is pass as a char*
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39 | // c) The new spectrum is pass as a "interpreted function", i.e., a
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40 | // function defined inside a ROOT macro, which will be invoked by the
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41 | // ROOT Cint itself. This is the case when we use ROOT macros.
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42 | // d) The new spectrum is pass as a "real function", i.e., a
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43 | // function defined inside normal c++ file.
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44 | //
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45 | // Method:
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46 | // ------
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47 | //
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48 | // -Corsika spectrun: dN/dE = A * E^(a)
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49 | // with a = fCorsikaSlope, and A = N/integral{E*de} from ELowLim to EUppLim
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50 | //
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51 | // -New spectrum: dN/dE = B * g(E)
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52 | // where B = N/integral{g*dE} from ELowLim to EUppLim, and N=NumEvents
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53 | //
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54 | // For converting the spectrum simulated with Corsika to the new one, we apply
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55 | // a weight to each event, given by:
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56 | //
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57 | // W(E) = B/A * g(E)/E^(a)
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58 | //
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59 | // In the case the new spectrum is simply a power law: dN/dE = B * E^(b), we
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60 | // have:
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61 | //
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62 | // W(E) = B/A * E^(b-a)
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63 | //
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64 | // (The factor B/A is used in order both the original and new spectrum have
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65 | // the same area (i.e. in order they represent the same number of showers))
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66 | //
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67 | // Note:
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68 | // ------
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69 | // -If the the new spectrum is just a power law (i.e. the user only specify
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70 | // the slope), the needed calculations (such as the integral of the
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71 | // spectrum) are done analytically. But if the new spectrum is given as a
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72 | // TF1 object, the calculations is done numerically.
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73 | //
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74 | // ToDo:
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75 | // -----
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76 | // -Give to the user also the possibility to specify the integral of the
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77 | // spectrum as another TF1 object (or C++ function)
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78 | //
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79 | //
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80 | // Input Containers:
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81 | // MMcEvt, MMcRunHeader, MMcCorsikaRunHeader
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82 | //
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83 | // Output Container:
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84 | // MWeight
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85 | //
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86 | //////////////////////////////////////////////////////////////////////////////
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87 |
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88 | #include "MMcWeightEnergySpecCalc.h"
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89 |
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90 | #include "MParList.h"
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91 | #include "MLog.h"
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92 | #include "MLogManip.h"
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93 | #include "MMcEvt.hxx"
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94 | #include "MMcRunHeader.hxx"
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95 | #include "MMcCorsikaRunHeader.h"
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96 | #include "MWeight.h"
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97 |
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98 | #include "TF1.h"
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99 | #include "TGraph.h"
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100 |
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101 | ClassImp(MMcWeightEnergySpecCalc);
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102 |
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103 | using namespace std;
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104 |
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105 |
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106 |
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107 | void MMcWeightEnergySpecCalc::Init(const char *name, const char *title)
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108 | {
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109 |
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110 | fName = name ? name : "MMcWeightEnergySpecCalc";
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111 | fTitle = title ? title : "Task to calculate weights to change the energy spectrum";
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112 |
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113 | AddToBranchList("MMcEvt.fEnergy");
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114 |
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115 | fAllEvtsTriggered = kFALSE;
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116 | fTotalNumSimulatedShowers = 0;
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117 | }
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118 |
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119 |
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120 | // ---------------------------------------------------------------------------
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121 | //
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122 | // Constructor. The new spectrum will be just a power law.
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123 | //
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124 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(Float_t slope,
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125 | const char *name, const char *title)
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126 | {
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127 | fNewSpecIsPowLaw = kTRUE;
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128 | fNewSlope = slope;
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129 |
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130 | fNewSpectrum = NULL;
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131 |
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132 | Init(name,title);
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133 | }
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134 |
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135 | // ---------------------------------------------------------------------------
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136 | //
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137 | // Constructor. The new spectrum will have a general shape, given by the user
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138 | // as a TF1 function.
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139 | //
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140 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(const TF1& spectrum,
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141 | const char *name, const char *title)
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142 | {
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143 | fNewSpecIsPowLaw = kFALSE;
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144 | fNewSpectrum = (TF1*)spectrum.Clone();
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145 |
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146 | Init(name,title);
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147 | }
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148 |
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149 | // ---------------------------------------------------------------------------
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150 | //
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151 | // As before, but the function which represent the new spectrum is given as
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152 | // a char* . Starting from it, we build a TF1 function
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153 | //
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154 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(const char* spectrum,
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155 | const char *name, const char *title)
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156 | {
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157 | fNewSpecIsPowLaw = kFALSE;
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158 | fNewSpectrum = new TF1("NewSpectrum",spectrum);
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159 |
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160 | Init(name,title);
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161 | }
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162 |
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163 | // ---------------------------------------------------------------------------
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164 | //
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165 | // As before, but the new spectrum is given as a intrepreted C++ function.
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166 | // Starting from it we build a TF1 function.
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167 | // This constructor is called for interpreted functions by CINT, i.e., when
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168 | // the functions are declared inside a ROOT macro.
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169 | //
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170 | // NOTE: you muss do a casting to (void*) of the function that you pass to this
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171 | // constructor before invoking it in a macro, e.g.
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172 | //
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173 | // Double_t myfunction(Double_t *x, Double_t *par)
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174 | // {
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175 | // ...
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176 | // }
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177 | //
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178 | // MMcWeightEnergySpecCalc wcalc((void*)myfunction);
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179 | //
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180 | // tasklist.AddToList(&wcalc);
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181 | //
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182 | // otherwise ROOT will invoke the constructor McWeightEnergySpecCalc(
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183 | // const char* spectrum, const char *name, const char *title)
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184 | //
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185 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(void* function,
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186 | const char *name, const char *title)
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187 | {
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188 | fNewSpecIsPowLaw = kFALSE;
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189 | fNewSpectrum = new TF1("NewSpectrum",function,0,1,1);
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190 |
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191 | Init(name,title);
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192 | }
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193 |
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194 | // ---------------------------------------------------------------------------
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195 | //
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196 | // As before, but this is the constructor for real functions, i.e. it is called
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197 | // when invoked with the normal C++ compiler, i.e. not inside a ROOT macro.
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198 | //
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199 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(Double_t (*function)(Double_t*x, Double_t* par), const Int_t npar, const char *name, const char *title)
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200 | {
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201 | fNewSpecIsPowLaw = kFALSE;
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202 | fNewSpectrum = new TF1("NewSpectrum",function,0,1,1);
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203 |
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204 | Init(name,title);
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205 | }
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206 |
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207 |
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208 |
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209 | // ----------------------------------------------------------------------------
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210 | //
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211 | // Destructor. Deletes the cloned fNewSpectrum.
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212 | //
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213 | MMcWeightEnergySpecCalc::~MMcWeightEnergySpecCalc()
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214 | {
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215 | if (fNewSpectrum)
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216 | delete fNewSpectrum;
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217 | }
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218 |
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219 |
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220 |
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221 | // ---------------------------------------------------------------------------
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222 | //
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223 | //
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224 | Int_t MMcWeightEnergySpecCalc::PreProcess (MParList *pList)
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225 | {
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226 |
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227 | fMcEvt = (MMcEvt*)pList->FindObject("MMcEvt");
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228 | if (!fMcEvt)
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229 | {
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230 | *fLog << err << dbginf << "MMcEvt not found... exit." << endl;
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231 | return kFALSE;
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232 | }
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233 |
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234 | fWeight = (MWeight*)pList->FindCreateObj("MWeight");
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235 | if (!fWeight)
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236 | {
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237 | *fLog << err << dbginf << "MWeight not found... exit." << endl;
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238 | return kFALSE;
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239 | }
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240 |
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241 | return kTRUE;
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242 | }
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243 |
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244 |
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245 |
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246 | // ----------------------------------------------------------------------------
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247 | //
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248 | // Executed each time a new root file is loaded
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249 | // We will need fCorsikaSlope and fE{Upp,Low}Lim to calculate the weights
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250 | //
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251 | Bool_t MMcWeightEnergySpecCalc::ReInit(MParList *plist)
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252 | {
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253 | MMcRunHeader *runheader = (MMcRunHeader*)plist->FindObject("MMcRunHeader");
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254 | if (!runheader)
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255 | {
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256 | *fLog << err << dbginf << "Error - MMcRunHeader not found... exit." << endl;
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257 | return kFALSE;
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258 | }
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259 |
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260 | MMcCorsikaRunHeader *corrunheader = (MMcCorsikaRunHeader*)plist->FindObject("MMcCorsikaRunHeader");
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261 | if (!corrunheader)
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262 | {
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263 | *fLog << err << dbginf << "Error - MMcCorsikaRunHeader not found... exit." << endl;
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264 | return kFALSE;
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265 | }
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266 |
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267 |
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268 | fCorsikaSlope = (Double_t)corrunheader->GetSlopeSpec();
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269 | fELowLim = (Double_t)corrunheader->GetELowLim();
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270 | fEUppLim = (Double_t)corrunheader->GetEUppLim();
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271 |
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272 | fTotalNumSimulatedShowers += runheader->GetNumSimulatedShowers();
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273 | fAllEvtsTriggered |= runheader->GetAllEvtsTriggered();
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274 |
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275 |
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276 |
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277 | *fLog << inf << "Slope of primaries' energy spectrum of Simulated showers: " << fCorsikaSlope << endl;
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278 | *fLog << inf << "Limits of energy range of Simulated showers: "
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279 | << fELowLim <<" - " << fEUppLim << endl;
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280 | *fLog << inf << "New Slope for Simulated showers: " << fNewSlope << endl;
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281 | *fLog << inf << "Total Number of Simulated showers: "
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282 | << fTotalNumSimulatedShowers << endl;
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283 | *fLog << inf << "Only triggered events avail: " << (fAllEvtsTriggered?"yes":"no") << endl;
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284 |
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285 |
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286 |
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287 | //
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288 | // Sanity checks to be sure that we won't divide by zero later on
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289 | //
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290 | if(fCorsikaSlope == -1. || fNewSlope == -1.)
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291 | {
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292 | *fLog << err << "The Slope of the power law must be different of -1... exit" << endl;
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293 | return kFALSE;
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294 | }
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295 |
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296 |
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297 | //
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298 | // Starting from fCorsikaSlope and fE{Upp,Low}Lim, calculate the integrals
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299 | // of both, the original Corsika spectrum and the new one.
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300 | //
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301 | //
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302 | // For the Corsika simulated spectrum (just a power law), we have:
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303 | //
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304 | fCorSpecInt = ( pow(fEUppLim,1+fCorsikaSlope) - pow(fELowLim,1+fCorsikaSlope) ) / ( 1+fCorsikaSlope );
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305 |
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306 |
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307 | //
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308 | // For the new spectrum:
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309 | //
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310 | if (fNewSpecIsPowLaw) // just the integral of a power law
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311 | {
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312 | fNewSpecInt = ( pow(fEUppLim,1+fNewSlope) - pow(fELowLim,1+fNewSlope) )/ ( 1+fNewSlope );
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313 | }
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314 | else
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315 | {
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316 | fNewSpectrum->SetRange(fELowLim, fEUppLim);
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317 |
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318 | // In this case we have to integrate the new spectrum numerically. We
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319 | // could do simply fNewSpectrum->Integral(fELowLim,fEUppLim), but ROOT
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320 | // fails integrating up to fEUppLim for a sharp cutoff spectrum
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321 |
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322 | //
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323 | // Trick to calculate the integral numerically (it works better than
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324 | // fNewSpectrum->Integral(fELowLim,fEUppLim) (although not perfectlly)
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325 | //
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326 | fNewSpectrum->SetNpx(1000);
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327 | TGraph gr(fNewSpectrum,"i");
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328 | Int_t Npx = gr.GetN();
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329 | Double_t* y = gr.GetY();
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330 |
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331 | const Double_t integral = y[Npx-1];
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332 | fNewSpecInt = integral;
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333 | }
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334 |
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335 |
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336 | return kTRUE;
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337 | }
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338 |
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339 |
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340 |
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341 | // ----------------------------------------------------------------------------
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342 | //
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343 | //
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344 | Int_t MMcWeightEnergySpecCalc::Process()
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345 | {
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346 | const Double_t energy = fMcEvt->GetEnergy();
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347 |
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348 | const Double_t C = fCorSpecInt / fNewSpecInt;
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349 | Double_t weight;
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350 |
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351 |
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352 | if (fNewSpecIsPowLaw)
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353 | weight = C * pow(energy,fNewSlope-fCorsikaSlope);
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354 | else
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355 | weight = C * fNewSpectrum->Eval(energy) / pow(energy,fCorsikaSlope);
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356 |
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357 |
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358 | fWeight->SetWeight( weight );
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359 |
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360 | return kTRUE;
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361 | }
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