source: trunk/MagicSoft/Simulation/Detector/ReflectorII/Changelog@ 1908

Last change on this file since 1908 was 1908, checked in by moralejo, 21 years ago
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1** Add changes at the beginning! **
2
34/04/2003 A. Moralejo
4
5init.h, geometry.c, ph2cph.c:
6introduced variable ct_max_radius, the maximum distance in x or y from the
7center to the edge of the telescope, measured on the parabolic dish. This
8is used in a fast check of whether the photon hits the disk in ph2cph.c
9
10ph2cph.c:
11in function Lin2Curv(float x), changed the calculation of the curvilinear
12coordinates (which before was only valid for ~17 m focus paraboloids).
13
1422/01/2003 A. Moralejo
15
16Fixed small bug in reflector.c. The end of run flag was not written to the
17output when the max_events option was used in the input card.
18
1921/01/2003 A. Moralejo
20
21Removed from the output a null byte written right after the ascii label
22containing the program version number which is at the beginning of the rfl
23file.
24
2519/12/2002 - 17/01/2003 A. Moralejo
26
27Lots of changes. Moved simulation of Mie scattering and Ozone absorption from
28attenu.f to atm.c, and changed the way it is done. Before it was not correct
29for large zenith angle (a variation like for Rayleigh scattering was assumed
30for both Mie scattering and Ozone absorption).
31
32
3313/12/2002 A. Moralejo
34
35attenu.f: Found mistake in Mie absorption calculation (height from sea
36level was taken as height above observation level). Changed optical depths
37table for Mie attenuation. Now they are no longer referred to 2 km height,
38but to sea level. Detector level is taken into account later in calculation.
39
4010/12/2002 A. Moralejo
41
42attenu.f: Added comments, removed old/unnecessary code, corrected small
43mistake in Elterman's table for ozone optical depth.
44
45atm.c,h : removed atmospheric model "ATM_ISOTHERMAL" which actually was
46not even implemented in the code, although it could be selected in the
47input card.
48
4915/11/2002 A. Moralejo
50
51ph2cph.c: Fixed BUG in timing calculation!!! The time to be subtracted
52(mirror till ground) had the wrong sign!!!
53
54reflector.c: in the wavelength range check, changed the range limits to
55the fixed values 290 and 600 nm. The StarFieldAdder cer files could not be
56processed otherwise, because the w range is not written in their headers.
57
58ph2cph.c: changed sign of phi angle to make it positive. This was necessary
59since now the vector indicating the reflected photon trajectory has also
60changed sign! (see note below, 11/11).
61
6214/11/2002 A. Moralejo
63reflector.c, parms.c: Added wobble mode option. Added wobble flag to the
64output and also an atmospheric_model flag.
65
6613/11/2002 A. Moralejo
67reflector.c, header.h: Introduced 3 counters to keep track of what proportion
68of the C-photons in each event have been produced by electrons, muons or
69other particles.
70
7111/11/2002 A. Moralejo
72ph2cph.c: BUG found! and fixed: the direction cosines in the cer files are
73those of the downgoing directions of photons, hence third component is
74negative. Before it was assumed positive. This, together with a wrong
75reflection in the individual mirrors (also changed) resulted in a subtle
76error which produced a quite de-focused reflector!
77
78reflector.c: for the same reason as above, the sign of theta in the calls
79to makeOmega had to be changed (+pi added to the phi argument).
80
81geometry.c, ph2cph.c, reflector.c, init.h: eliminated array ct_Focal[]
82which contained the focal lengths of individual mirrors. It was redundant
83since the same information is available in ct_data[].f
84
85Oct/2002 A. Moralejo
86added attach.c to attach the files magic.def, axisdev.dat and
87reflectivity.dat to the end of the reflector output.
88
89Sept/2002 A. Moralejo
90header.h, reflector.c: added run header (=Corsika's), changed event header.
91
923/7/2002 A. Moralejo
93reflector.c: Introduced NaN check in the photon loop.
94If NAns are found in a photon data block, it is not processed.
95
96ph2cph.c: Introduced "check of positiveness" before taking the sqrt
97in the calculation of the photon trajectory intersection with the
98global paraboloid.
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