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