1 | ** Add changes at the beginning! **
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2 |
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3 | 4/04/2003 A. Moralejo
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4 |
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5 | init.h, geometry.c, ph2cph.c:
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6 | introduced variable ct_max_radius, the maximum distance in x or y from the
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7 | center to the edge of the telescope, measured on the parabolic dish. This
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8 | is used in a fast check of whether the photon hits the disk in ph2cph.c
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9 |
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10 | ph2cph.c:
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11 | in function Lin2Curv(float x), changed the calculation of the curvilinear
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12 | coordinates (which before was only valid for ~17 m focus paraboloids).
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13 |
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14 | 22/01/2003 A. Moralejo
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15 |
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16 | Fixed small bug in reflector.c. The end of run flag was not written to the
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17 | output when the max_events option was used in the input card.
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18 |
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19 | 21/01/2003 A. Moralejo
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20 |
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21 | Removed from the output a null byte written right after the ascii label
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22 | containing the program version number which is at the beginning of the rfl
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23 | file.
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24 |
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25 | 19/12/2002 - 17/01/2003 A. Moralejo
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26 |
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27 | Lots of changes. Moved simulation of Mie scattering and Ozone absorption from
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28 | attenu.f to atm.c, and changed the way it is done. Before it was not correct
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29 | for large zenith angle (a variation like for Rayleigh scattering was assumed
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30 | for both Mie scattering and Ozone absorption).
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31 |
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32 |
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33 | 13/12/2002 A. Moralejo
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34 |
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35 | attenu.f: Found mistake in Mie absorption calculation (height from sea
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36 | level was taken as height above observation level). Changed optical depths
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37 | table for Mie attenuation. Now they are no longer referred to 2 km height,
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38 | but to sea level. Detector level is taken into account later in calculation.
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39 |
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40 | 10/12/2002 A. Moralejo
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41 |
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42 | attenu.f: Added comments, removed old/unnecessary code, corrected small
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43 | mistake in Elterman's table for ozone optical depth.
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44 |
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45 | atm.c,h : removed atmospheric model "ATM_ISOTHERMAL" which actually was
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46 | not even implemented in the code, although it could be selected in the
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47 | input card.
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48 |
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49 | 15/11/2002 A. Moralejo
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50 |
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51 | ph2cph.c: Fixed BUG in timing calculation!!! The time to be subtracted
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52 | (mirror till ground) had the wrong sign!!!
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53 |
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54 | reflector.c: in the wavelength range check, changed the range limits to
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55 | the fixed values 290 and 600 nm. The StarFieldAdder cer files could not be
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56 | processed otherwise, because the w range is not written in their headers.
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57 |
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58 | ph2cph.c: changed sign of phi angle to make it positive. This was necessary
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59 | since now the vector indicating the reflected photon trajectory has also
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60 | changed sign! (see note below, 11/11).
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61 |
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62 | 14/11/2002 A. Moralejo
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63 | reflector.c, parms.c: Added wobble mode option. Added wobble flag to the
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64 | output and also an atmospheric_model flag.
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65 |
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66 | 13/11/2002 A. Moralejo
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67 | reflector.c, header.h: Introduced 3 counters to keep track of what proportion
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68 | of the C-photons in each event have been produced by electrons, muons or
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69 | other particles.
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70 |
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71 | 11/11/2002 A. Moralejo
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72 | ph2cph.c: BUG found! and fixed: the direction cosines in the cer files are
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73 | those of the downgoing directions of photons, hence third component is
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74 | negative. Before it was assumed positive. This, together with a wrong
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75 | reflection in the individual mirrors (also changed) resulted in a subtle
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76 | error which produced a quite de-focused reflector!
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77 |
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78 | reflector.c: for the same reason as above, the sign of theta in the calls
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79 | to makeOmega had to be changed (+pi added to the phi argument).
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80 |
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81 | geometry.c, ph2cph.c, reflector.c, init.h: eliminated array ct_Focal[]
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82 | which contained the focal lengths of individual mirrors. It was redundant
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83 | since the same information is available in ct_data[].f
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84 |
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85 | Oct/2002 A. Moralejo
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86 | added attach.c to attach the files magic.def, axisdev.dat and
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87 | reflectivity.dat to the end of the reflector output.
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88 |
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89 | Sept/2002 A. Moralejo
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90 | header.h, reflector.c: added run header (=Corsika's), changed event header.
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91 |
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92 | 3/7/2002 A. Moralejo
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93 | reflector.c: Introduced NaN check in the photon loop.
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94 | If NAns are found in a photon data block, it is not processed.
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95 |
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96 | ph2cph.c: Introduced "check of positiveness" before taking the sqrt
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97 | in the calculation of the photon trajectory intersection with the
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98 | global paraboloid.
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99 |
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100 |
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101 |
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