1 | ** Add changes at the beginning! **
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2 |
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3 | 28/08/2004 A. Moralejo
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4 |
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5 | Changes in configuration files. Renamed Data/magic.def and Data/axisdev.dat
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6 | to magic_no_chessboard.def and axisdev_no_chessboard.def. Now default
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7 | axisdev.dat and magic.def contain 964 mirrors as in the present MAGIC
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8 | configuration, and the panels are in a chessboard pattern
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9 |
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10 | 30/04/2003 A. Moralejo
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11 |
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12 | ph2cph.c: Found out that the fix from yesterday, although it "patched" the
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13 | loss of photons, did not remove the real cause for it. Actually in the
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14 | determination of the intersection of the photon with the paraboloid there
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15 | was an overflow which resulted in nonsense coordinates beyond 10 m from
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16 | the mirror dish center. It has been fixed fixed by changing the following
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17 | cut:
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18 |
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19 | if ( fabs(a) < 1.e-3 ) {
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20 | xcut[2] = -c / b
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21 | }
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22 |
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23 | which was formerly < 1.e-6.
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24 |
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25 | I also noticed that the problem from yesterday was not so serious: it only
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26 | removed a significant amount of the photons nearly paralel to the telescope
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27 | axis, but globally, over a cer file there is no big difference.
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28 |
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29 | 29/04/2003 A. Moralejo
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30 |
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31 | ph2cph.c:
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32 | Changed determination of which mirror element is hit. Before there was a
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33 | problem when going to very large distances from the mirror center, sometimes
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34 | a wrong mirror was chosen, which was actually further away from the impact
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35 | point than the mirror size, and therefore the photon was discarded later as
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36 | "not hitting any mirror" (about 20% loss for eco1000) Now we measure the
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37 | distance on the paraboloid. The new code is:
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38 |
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39 | /* calculate the mirror to be used */
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40 |
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41 | distmirr = 1000000.0f;
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42 |
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43 | for (i=0; i<ct_NMirrors && distmirr>=ct_RMirror; ++i) {
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44 | distmirr2 = (float) sqrt(SQR(ct_data[i].sx - sx) +
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45 | SQR(ct_data[i].sy - sy));
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46 |
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47 | if (distmirr2 < distmirr) {
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48 | i_mirror = i;
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49 | distmirr = distmirr2;
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50 | }
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51 | }
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52 |
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53 | Now the "distance" we calculate on the paraboloid is not a real distance,
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54 | because sx,sy are measured along the cut between the paraboloid and planes
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55 | containing the paraboloid axis and the x or y axis... but this should not
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56 | matter much with such "flat" paraboloids. What cannot be done, as was before,
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57 | is check the distance in the x,y,z space and then check whether the photon
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58 | is inside the mirror in the sx,sy space, because then we lose photons for
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59 | which a nearest mirror is chosen which in sx,sy is not close enough to
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60 | contain the photon.
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61 |
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62 | geometry.c:
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63 | Small change in calculation of ct_nax_radius (introduced fabs, but nothing
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64 | changes)
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65 |
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66 | 16/04/2003 A. Moralejo
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67 |
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68 | MagicSoft/Simulation/Detector/Data/ :
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69 | Added eco1000.def and axisdev1000.dat for eco-1000 studies
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70 |
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71 | 4/04/2003 A. Moralejo
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72 |
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73 | init.h, geometry.c, ph2cph.c:
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74 | introduced variable ct_max_radius, the maximum distance in x or y from the
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75 | center to the edge of the telescope, measured on the parabolic dish. This
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76 | is used in a fast check of whether the photon hits the disk in ph2cph.c
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77 |
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78 | ph2cph.c:
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79 | in function Lin2Curv(float x), changed the calculation of the curvilinear
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80 | coordinates (which before was only valid for ~17 m focus paraboloids).
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81 |
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82 | 22/01/2003 A. Moralejo
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83 |
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84 | Fixed small bug in reflector.c. The end of run flag was not written to the
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85 | output when the max_events option was used in the input card.
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86 |
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87 | 21/01/2003 A. Moralejo
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88 |
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89 | Removed from the output a null byte written right after the ascii label
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90 | containing the program version number which is at the beginning of the rfl
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91 | file.
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92 |
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93 | 19/12/2002 - 17/01/2003 A. Moralejo
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94 |
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95 | Lots of changes. Moved simulation of Mie scattering and Ozone absorption from
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96 | attenu.f to atm.c, and changed the way it is done. Before it was not correct
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97 | for large zenith angle (a variation like for Rayleigh scattering was assumed
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98 | for both Mie scattering and Ozone absorption).
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99 |
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100 |
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101 | 13/12/2002 A. Moralejo
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102 |
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103 | attenu.f: Found mistake in Mie absorption calculation (height from sea
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104 | level was taken as height above observation level). Changed optical depths
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105 | table for Mie attenuation. Now they are no longer referred to 2 km height,
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106 | but to sea level. Detector level is taken into account later in calculation.
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107 |
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108 | 10/12/2002 A. Moralejo
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109 |
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110 | attenu.f: Added comments, removed old/unnecessary code, corrected small
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111 | mistake in Elterman's table for ozone optical depth.
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112 |
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113 | atm.c,h : removed atmospheric model "ATM_ISOTHERMAL" which actually was
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114 | not even implemented in the code, although it could be selected in the
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115 | input card.
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116 |
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117 | 15/11/2002 A. Moralejo
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118 |
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119 | ph2cph.c: Fixed BUG in timing calculation!!! The time to be subtracted
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120 | (mirror till ground) had the wrong sign!!!
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121 |
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122 | reflector.c: in the wavelength range check, changed the range limits to
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123 | the fixed values 290 and 600 nm. The StarFieldAdder cer files could not be
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124 | processed otherwise, because the w range is not written in their headers.
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125 |
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126 | ph2cph.c: changed sign of phi angle to make it positive. This was necessary
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127 | since now the vector indicating the reflected photon trajectory has also
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128 | changed sign! (see note below, 11/11).
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129 |
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130 | 14/11/2002 A. Moralejo
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131 | reflector.c, parms.c: Added wobble mode option. Added wobble flag to the
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132 | output and also an atmospheric_model flag.
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133 |
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134 | 13/11/2002 A. Moralejo
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135 | reflector.c, header.h: Introduced 3 counters to keep track of what proportion
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136 | of the C-photons in each event have been produced by electrons, muons or
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137 | other particles.
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138 |
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139 | 11/11/2002 A. Moralejo
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140 | ph2cph.c: BUG found! and fixed: the direction cosines in the cer files are
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141 | those of the downgoing directions of photons, hence third component is
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142 | negative. Before it was assumed positive. This, together with a wrong
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143 | reflection in the individual mirrors (also changed) resulted in a subtle
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144 | error which produced a quite de-focused reflector!
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145 |
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146 | reflector.c: for the same reason as above, the sign of theta in the calls
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147 | to makeOmega had to be changed (+pi added to the phi argument).
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148 |
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149 | geometry.c, ph2cph.c, reflector.c, init.h: eliminated array ct_Focal[]
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150 | which contained the focal lengths of individual mirrors. It was redundant
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151 | since the same information is available in ct_data[].f
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152 |
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153 | Oct/2002 A. Moralejo
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154 | added attach.c to attach the files magic.def, axisdev.dat and
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155 | reflectivity.dat to the end of the reflector output.
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156 |
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157 | Sept/2002 A. Moralejo
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158 | header.h, reflector.c: added run header (=Corsika's), changed event header.
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159 |
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160 | 3/7/2002 A. Moralejo
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161 | reflector.c: Introduced NaN check in the photon loop.
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162 | If NAns are found in a photon data block, it is not processed.
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163 |
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164 | ph2cph.c: Introduced "check of positiveness" before taking the sqrt
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165 | in the calculation of the photon trajectory intersection with the
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166 | global paraboloid.
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167 |
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168 |
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169 |
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