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 expressed
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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): Thomas Bretz, 3/2004 <mailto:tbretz@astro.uni-wuerzburg.de>
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19 | ! Author(s): Robert Wagner, 7/2004 <mailto:rwagner@mppmu.mpg.de>
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20 | !
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21 | ! Copyright: MAGIC Software Development, 2000-2004
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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 | //
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28 | // MAstroCamera
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29 | // ============
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30 | //
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31 | // A tools displaying stars from a catalog in the camera display.
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32 | // PRELIMINARY!!
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33 | //
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34 | //
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35 | // Usage:
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36 | // ------
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37 | // For a usage example see macros/starfield.C
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38 | //
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39 | // To be able to reflect the star-light you need the geometry of the
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40 | // mirror and the distance of the plain screen.
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41 | //
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42 | // You can get the mirror geometry from a MC file and the distance of
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43 | // the screen from MGeomCam.
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44 | //
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45 | //
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46 | // Algorithm:
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47 | // ----------
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48 | // The calculation of the position of the reflection in the camera is
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49 | // done by:
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50 | // - Rotation of the star-field such that the camera is looking into
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51 | // the pointing direction
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52 | // - Calculation of the reflected star-light vector by calling
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53 | // MGeomMirror::GetReflection (which returns the point at which
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54 | // the vector hits the camera plain)
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55 | // - Depending on the draw-option you get each reflected point, the
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56 | // reflection on a virtual ideal mirror or the reflection on each
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57 | // individual mirror
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58 | //
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59 | //
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60 | // GUI:
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61 | // ----
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62 | // * You can use the the cursor keys to change the pointing position
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63 | // and plus/minus to change the time by a quarter of an hour.
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64 | //
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65 | // ToDo:
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66 | // -----
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67 | // * possibility to overwrite distance from mirror to screen
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68 | // * read the mirror geometry directly from the MC input file
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69 | //
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70 | /////////////////////////////////////////////////////////////////////////////
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71 | #include "MAstroCamera.h"
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72 |
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73 | #include <errno.h> // strerror
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74 | #include <fstream> // ifstream
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75 |
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76 | #include <KeySymbols.h> // kKey_*
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77 |
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78 | #include <TH2.h> // TH2D
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79 | #include <TMarker.h> // TMarker
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80 | #include <TVirtualPad.h> // gPad
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81 |
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82 | #include "MLog.h"
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83 | #include "MLogManip.h"
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84 |
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85 | #include "MGeomCam.h"
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86 | #include "MGeomMirror.h"
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87 |
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88 | #include "MTime.h"
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89 | #include "MAstroSky2Local.h"
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90 | #include "MObservatory.h"
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91 |
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92 | #include "../mhist/MHCamera.h" // FIXME: This dependancy is very bad!
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93 | // HOW TO GET RID OF IT? Move MHCamera to mgeom?
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94 |
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95 | #include "MStarPos.h"
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96 |
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97 | ClassImp(MAstroCamera);
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98 |
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99 | using namespace std;
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100 |
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101 | // --------------------------------------------------------------------------
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102 | //
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103 | // Create a virtual MGeomMirror which is in the center of the coordinate
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104 | // system and has a normal vector in z-direction.
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105 | //
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106 | MAstroCamera::MAstroCamera() : fGeom(0), fMirrors(0)
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107 | {
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108 | fMirror0 = new MGeomMirror;
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109 | fMirror0->SetMirrorContent(0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1);
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110 | }
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111 |
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112 | // --------------------------------------------------------------------------
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113 | //
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114 | // Delete fGeom, fMirrors and the virtual 0-Mirror fMirror0
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115 | //
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116 | MAstroCamera::~MAstroCamera()
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117 | {
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118 | if (fGeom)
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119 | delete fGeom;
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120 | if (fMirrors)
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121 | delete fMirrors;
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122 |
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123 | delete fMirror0;
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124 |
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125 | }
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126 |
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127 | // --------------------------------------------------------------------------
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128 | //
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129 | // Set a list of mirrors. The Mirrors must be of type MGeomMirror and
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130 | // stored in a TClonesArray
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131 | //
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132 | void MAstroCamera::SetMirrors(TClonesArray &arr)
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133 | {
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134 | if (arr.GetClass()!=MGeomMirror::Class())
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135 | {
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136 | cout << "ERROR - TClonesArray doesn't contain objects of type MGeomMirror... ignored." << endl;
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137 | return;
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138 | }
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139 |
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140 | const Int_t n = arr.GetSize();
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141 |
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142 | if (!fMirrors)
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143 | fMirrors = new TClonesArray(MGeomMirror::Class(), n);
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144 |
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145 | fMirrors->ExpandCreate(n);
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146 |
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147 | for (int i=0; i<n; i++)
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148 | memcpy((*fMirrors)[i], arr[i], sizeof(MGeomMirror));
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149 |
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150 | }
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151 |
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152 |
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153 | // --------------------------------------------------------------------------
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154 | //
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155 | // Read the mirror geometry from a MC .def file. The following
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156 | // structure is expected:
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157 | //
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158 | // #* TYPE=1 (MAGIC)
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159 | // #* i f sx sy x y z thetan phin
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160 | // #*
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161 | // #* i : number of the mirror
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162 | // #* f : focal distance of that mirror
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163 | // #* sx : curvilinear coordinate of mirror's center in X[cm]
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164 | // #* sy : curvilinear coordinate of mirror's center in X[cm]
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165 | // #* x : x coordinate of the center of the mirror [cm]
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166 | // #* y : y coordinate of the center of the mirror [cm]
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167 | // #* z : z coordinate of the center of the mirror [cm]
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168 | // #* thetan : polar theta angle of the direction where the mirror points to
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169 | // #* phin : polar phi angle of the direction where the mirror points to
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170 | // #* xn : xn coordinate of the normal vector in the center (normalized)
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171 | // #* yn : yn coordinate of the normal vector in the center (normalized)
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172 | // #* zn : zn coordinate of the normal vector in the center (normalized)
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173 | // #
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174 | // define_mirrors
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175 | // 1 1700.9200 25.0002 75.0061 25.0000 75.0000 0.9207 0.02328894 1.24904577 -0.00736394 -0.02209183 0.99972882
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176 | // 2 ...
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177 | //
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178 | void MAstroCamera::SetMirrors(const char *fname)
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179 | {
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180 | ifstream fin(fname);
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181 | if (!fin)
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182 | {
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183 | gLog << err << "Cannot open file " << fname << ": ";
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184 | gLog << strerror(errno) << endl;
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185 | return;
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186 | }
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187 |
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188 | TString line;
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189 | while (1)
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190 | {
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191 | line.ReadLine(fin);
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192 | if (!fin)
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193 | return;
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194 |
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195 | line = line.Strip(TString::kBoth);
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196 |
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197 | if (line.BeginsWith("n_mirrors"))
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198 | {
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199 | Int_t n;
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200 | sscanf(line.Data(), "%*s %d", &n);
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201 |
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202 | if (!fMirrors)
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203 | fMirrors = new TClonesArray(MGeomMirror::Class(), n);
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204 |
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205 | fMirrors->ExpandCreate(n);
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206 | continue;
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207 | }
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208 |
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209 |
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210 | Int_t id;
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211 | Float_t f, sx, sy, x, y, z, thetan, phin, xn, yn, zn;
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212 |
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213 | const Int_t n = sscanf(line.Data(), "%d %f %f %f %f %f %f %f %f %f %f %f",
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214 | &id, &f, &sx, &sy, &x, &y, &z, &thetan,
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215 | &phin, &xn, &yn, &zn);
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216 | if (n!=12)
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217 | continue;
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218 |
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219 | new ((*fMirrors)[id-1]) MGeomMirror;
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220 | ((MGeomMirror*)(*fMirrors)[id-1])->SetMirrorContent(id, f, sx, sy, x, y, z, thetan, phin, xn, yn, zn);
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221 | }
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222 | }
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223 |
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224 | // --------------------------------------------------------------------------
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225 | //
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226 | // Set the camera geometry. The MGeomCam object is cloned.
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227 | //
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228 | void MAstroCamera::SetGeom(const MGeomCam &cam)
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229 | {
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230 | if (fGeom)
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231 | delete fGeom;
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232 |
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233 | fGeom = (MGeomCam*)cam.Clone();
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234 | }
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235 |
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236 | // --------------------------------------------------------------------------
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237 | //
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238 | // Convert To Pad coordinates (see MAstroCatalog)
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239 | //
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240 | Int_t MAstroCamera::ConvertToPad(const TVector3 &w, TVector2 &v) const
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241 | {
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242 | /*
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243 | --- Use this to plot the 'mean grid' instead of the grid of a
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244 | theoretical central mirror ---
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245 |
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246 | TVector3 spot;
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247 | const Int_t num = fConfig->GetNumMirror();
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248 | for (int i=0; i<num; i++)
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249 | spot += fConfig->GetMirror(i).GetReflection(w, fGeom->GetCameraDist())*1000;
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250 | spot *= 1./num;
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251 | */
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252 |
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253 | const TVector3 spot = fMirror0->GetReflection(w, fGeom->GetCameraDist())*1000;
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254 | v.Set(spot(0), spot(1));
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255 |
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256 | const Float_t max = fGeom->GetMaxRadius()*0.70;
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257 | return v.X()>-max && v.Y()>-max && v.X()<max && v.Y()<max;
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258 | }
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259 |
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260 | // --------------------------------------------------------------------------
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261 | //
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262 | // Find an object with a given name in the list of primitives of this pad.
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263 | //
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264 | TObject *FindObjectInPad(const char *name, TVirtualPad *pad)
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265 | {
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266 | if (!pad)
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267 | pad = gPad;
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268 |
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269 | if (!pad)
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270 | return NULL;
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271 |
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272 | TObject *o;
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273 |
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274 | TIter Next(pad->GetListOfPrimitives());
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275 | while ((o=Next()))
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276 | {
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277 | if (o->InheritsFrom(gROOT->GetClass(name)))
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278 | return o;
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279 |
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280 | if (o->InheritsFrom("TPad"))
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281 | if ((o = FindObjectInPad(name, (TVirtualPad*)o)))
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282 | return o;
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283 | }
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284 | return NULL;
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285 | }
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286 |
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287 | // --------------------------------------------------------------------------
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288 | //
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289 | // Options:
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290 | //
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291 | // '*' Draw the mean of the reflections on all mirrors
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292 | // '.' Draw a dot for the reflection on each individual mirror
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293 | // 'h' To create a TH2D of the star-light which is displayed
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294 | // 'c' Use the underlaying MHCamera as histogram
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295 | // '0' Draw the reflection on a virtual perfect mirror
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296 | // '=' Draw '0' or '*' propotional to the star magnitude
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297 | //
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298 | // If the Pad contains an object MHCamera of type MHCamera it is used.
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299 | // Otherwise a new object is created.
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300 | //
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301 | void MAstroCamera::AddPrimitives(TString o)
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302 | {
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303 | if (!fTime || !fObservatory || !fMirrors)
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304 | {
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305 | cout << "Missing data..." << endl;
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306 | return;
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307 | }
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308 |
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309 | if (o.IsNull())
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310 | o = "*.";
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311 |
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312 | const Bool_t hasnull = o.Contains("0", TString::kIgnoreCase);
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313 | const Bool_t hashist = o.Contains("h", TString::kIgnoreCase);
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314 | const Bool_t hasmean = o.Contains("*", TString::kIgnoreCase);
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315 | const Bool_t hasdot = o.Contains(".", TString::kIgnoreCase);
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316 | const Bool_t usecam = o.Contains("c", TString::kIgnoreCase);
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317 | const Bool_t resize = o.Contains("=", TString::kIgnoreCase);
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318 |
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319 | // Get camera
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320 | MHCamera *camera=(MHCamera*)FindObjectInPad("MHCamera", gPad);
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321 | if (camera)
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322 | {
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323 | if (!camera->GetGeometry() || camera->GetGeometry()->IsA()!=fGeom->IsA())
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324 | camera->SetGeometry(*fGeom);
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325 | }
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326 | else
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327 | {
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328 | camera = new MHCamera(*fGeom);
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329 | camera->SetName("MHCamera");
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330 | camera->SetStats(0);
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331 | camera->SetInvDeepBlueSeaPalette();
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332 | camera->SetBit(kCanDelete);
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333 | camera->Draw();
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334 | }
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335 |
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336 | camera->SetTitle(GetPadTitle());
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337 |
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338 | gPad->cd(1);
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339 |
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340 | if (!usecam)
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341 | {
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342 | if (camera->GetEntries()==0)
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343 | camera->SetBit(MHCamera::kNoLegend);
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344 | }
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345 | else
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346 | {
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347 | camera->Reset();
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348 | camera->SetYTitle("arb.cur");
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349 | }
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350 |
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351 | TH2 *h=0;
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352 | if (hashist)
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353 | {
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354 | TH2F hist("","", 90, -650, 650, 90, -650, 650);
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355 | hist.SetMinimum(0);
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356 | h = (TH2*)hist.DrawCopy("samecont1");
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357 | }
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358 |
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359 | const TRotation rot(GetGrid(kTRUE));
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360 |
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361 | MVector3 *radec;
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362 | TIter Next(&fList);
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363 |
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364 | while ((radec=(MVector3*)Next()))
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365 | {
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366 | const Double_t mag = radec->Magnitude();
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367 | if (mag>GetLimMag())
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368 | continue;
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369 |
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370 | TVector3 star(*radec);
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371 |
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372 | // Rotate Star into telescope system
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373 | star *= rot;
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374 |
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375 | TVector3 mean;
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376 |
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377 | Int_t num = 0;
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378 |
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379 | MGeomMirror *mirror = 0;
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380 | TIter NextM(fMirrors);
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381 | while ((mirror=(MGeomMirror*)NextM()))
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382 | {
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383 | const TVector3 spot = mirror->GetReflection(star, fGeom->GetCameraDist())*1000;
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384 |
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385 | // calculate mean of all 'stars' hitting the camera plane
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386 | // by taking the sum of the intersection points between
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387 | // the light vector and the camera plane
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388 | mean += spot;
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389 |
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390 | if (hasdot)
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391 | {
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392 | TMarker *m=new TMarker(spot(0), spot(1), 1);
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393 | TVector3 pos=mirror->GetMirrorCenter();
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394 | Float_t r=pos.Mag();
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395 |
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396 | m->SetMarkerColor((Int_t)(6*r)+51);
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397 | m->SetMarkerStyle(kDot);
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398 | fMapG.Add(m);
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399 | }
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400 | if (h)
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401 | h->Fill(spot(0), spot(1), pow(10, -mag/2.5));
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402 |
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403 | if (usecam)
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404 | camera->Fill(spot(0), spot(1), pow(10, -mag/2.5));
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405 |
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406 | num++;
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407 | }
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408 |
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409 | // transform meters into millimeters (camera display works with mm)
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410 | mean *= 1./num;
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411 | DrawStar(mean(0), mean(1), *radec, hasmean?kBlack:-1, Form("x=%.1fmm y=%.1fmm", mean(0), mean(1)), resize);
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412 | if (hasnull)
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413 | {
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414 | TVector3 star(*radec);
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415 | star *= rot;
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416 | const TVector3 spot = fMirror0->GetReflection(star, fGeom->GetCameraDist())*1000;
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417 | DrawStar(spot(0), spot(1), *radec, hasmean?kBlack:-1, Form("x=%.1fmm y=%.1fmm", mean(0), mean(1)), resize);
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418 | // This can be used to get the abberation...
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419 | //cout << TMath::Hypot(spot(0), spot(1)) << " " << TMath::Hypot(mean(0)-spot(0), mean(1)-spot(1)) << endl;
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420 | }
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421 | }
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422 | }
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423 |
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424 |
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425 | // --------------------------------------------------------------------------
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426 | //
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427 | // Fills a TList with all stars found under current presets
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428 | // (Coordinates, Time, FOV). The list is emptied before the filling is done.
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429 | // Currently, the mean spot when averaging over all mirrors is used.
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430 | //
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431 | void MAstroCamera::FillStarList(TList* list)
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432 | {
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433 | if (!fTime || !fObservatory || !fMirrors) {
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434 | cout << "Missing data..." << endl;
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435 | return;
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436 | }
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437 |
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438 | if (!list) {
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439 | cout << "Missing storage list for stars found..." << endl;
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440 | return;
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441 | }
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442 |
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443 | list->Delete(); // dump old list... (otherwise the same stars would pile up)
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444 |
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445 | const TRotation rot(GetGrid(kTRUE));
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446 | MVector3 *radec;
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447 | TIter Next(&fList);
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448 |
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449 | while ((radec=(MVector3*)Next())) {
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450 | const Double_t mag = radec->Magnitude();
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451 | if (mag>GetLimMag())
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452 | continue;
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453 | TVector3 star(*radec);
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454 | // Rotate Star into telescope system
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455 | star *= rot;
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456 | TVector3 mean;
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457 | Int_t num = 0;
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458 | MGeomMirror *mirror = 0;
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459 | TIter NextM(fMirrors);
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460 | while ((mirror=(MGeomMirror*)NextM())) {
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461 | const TVector3 spot = mirror->GetReflection(star, fGeom->GetCameraDist())*1000;
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462 | mean += spot;
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463 | num++;
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464 | }
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465 | mean *= 1./num;
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466 | MStarPos *starpos = new MStarPos;
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467 | starpos->SetExpValues(mag,mean(0),mean(1));
|
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468 |
|
---|
469 | const TVector3 spot = fMirror0->GetReflection(star, fGeom->GetCameraDist())*1000;
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470 | starpos->SetIdealValues(mag,spot(0),spot(1));
|
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471 | }
|
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472 | }
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473 |
|
---|
474 | // ------------------------------------------------------------------------
|
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475 | //
|
---|
476 | // Uses fRaDec as a reference point.
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477 | //
|
---|
478 | // Return dZd and dAz corresponding to the distance from x,y to fRaDec
|
---|
479 | //
|
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480 | // Before calling this function you should correct for abberation. In
|
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481 | // case of MAGIC you can do this by:
|
---|
482 | // x /= 1.0713;
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483 | // y /= 1.0713;
|
---|
484 | //
|
---|
485 | // x [mm]: x coordinate in the camera plane (assuming a perfect mirror)
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486 | // y [mm]: y coordinate in the camera plane (assuming a perfect mirror)
|
---|
487 | //
|
---|
488 | // We assume (0, 0) to be the center of the FOV
|
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489 | //
|
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490 | // dzd [deg]: Delta Zd
|
---|
491 | // daz [deg]: Delta Az
|
---|
492 | //
|
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493 | void MAstroCamera::GetDiffZdAz(Double_t x, Double_t y, Double_t &dzd, Double_t &daz)
|
---|
494 | {
|
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495 | // Reflect the corrected pixel on a perfect mirror
|
---|
496 | TVector3 v(x, y, fGeom->GetCameraDist()*1000);
|
---|
497 | TVector3 spot = fMirror0->GetReflection(v);
|
---|
498 |
|
---|
499 | // Derotate into the local coordinate system
|
---|
500 | const MAstroSky2Local rot(*fTime, *fObservatory);
|
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501 | const TRotation align(AlignCoordinates(rot*fRaDec).Inverse());
|
---|
502 | spot *= align;
|
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503 |
|
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504 | cout << "Zd="<<spot.Theta()*TMath::RadToDeg() << " ";
|
---|
505 | cout << "Az="<<spot.Phi() *TMath::RadToDeg()+360 << endl;
|
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506 |
|
---|
507 | // Derotatet the center of the camera
|
---|
508 | TVector3 c(0, 0, 1);
|
---|
509 | c *= align;
|
---|
510 |
|
---|
511 | dzd = (spot.Theta()-c.Theta())*TMath::RadToDeg();
|
---|
512 | daz = (spot.Phi() -c.Phi()) *TMath::RadToDeg();
|
---|
513 |
|
---|
514 | if (daz> 180) daz -= 360;
|
---|
515 | if (daz<-180) daz += 360;
|
---|
516 | }
|
---|
517 |
|
---|
518 | // ------------------------------------------------------------------------
|
---|
519 | //
|
---|
520 | // Execute a gui event on the camera
|
---|
521 | //
|
---|
522 | void MAstroCamera::ExecuteEvent(Int_t event, Int_t mp1, Int_t mp2)
|
---|
523 | {
|
---|
524 | // if (mp1>0 && mp2>0)
|
---|
525 | // {
|
---|
526 | // // Calculate World coordinates from pixel
|
---|
527 | // Double_t x = gPad->AbsPixeltoX(mp1);
|
---|
528 | // Double_t y = gPad->AbsPixeltoY(mp2);
|
---|
529 | //
|
---|
530 | // // Correct for abberation
|
---|
531 | // x /= 1.0713;
|
---|
532 | // y /= 1.0713;
|
---|
533 | //
|
---|
534 | // Double_t dzd, daz;
|
---|
535 | // GetDiffZdAz(x, y, dzd, daz);
|
---|
536 | //
|
---|
537 | // cout << "dZd="<< dzd << " " << "dAz="<< daz << endl;
|
---|
538 | // }
|
---|
539 | //
|
---|
540 | // For MAGIC the distance of the mean of the light distribution
|
---|
541 | // to the Mirror0 reflection of the star (Abberation) can be
|
---|
542 | // expressed as: dr = 0.0713*r = r/14.03
|
---|
543 | // +-0.0002
|
---|
544 |
|
---|
545 | if (event==kKeyPress && fTime)
|
---|
546 | switch (mp2)
|
---|
547 | {
|
---|
548 | case kKey_Plus:
|
---|
549 | fTime->SetMjd(fTime->GetMjd()+0.25/24);
|
---|
550 | Update(kTRUE);
|
---|
551 | return;
|
---|
552 |
|
---|
553 | case kKey_Minus:
|
---|
554 | fTime->SetMjd(fTime->GetMjd()-0.25/24);
|
---|
555 | Update(kTRUE);
|
---|
556 | return;
|
---|
557 | }
|
---|
558 |
|
---|
559 | MAstroCatalog::ExecuteEvent(event, mp1, mp2);
|
---|
560 | }
|
---|