source: trunk/MagicSoft/Simulation/Detector/Starfield/convertcorsika.cxx@ 353

Last change on this file since 353 was 341, checked in by petry, 25 years ago
First version of the Starfield Generator in this repository. Fully functional version using the SKY2000 star catalog.
File size: 2.8 KB
Line 
1//////////////////////////////////////////////////////////////////////////////////////
2// Write photon data in binary corsika-like format.
3// Output will be used as an input for the reflector as if it was a shower event.
4//
5//////////////////////////////////////////////////////////////////////////////////////
6
7#include "convertcorsika.h"
8
9COREventHeader cerevth;
10CORParticle cerphot;
11CORStatfile cerstat;
12
13int convertcorsika(int id, int photnum, photon phot[], float inttime_s, int verbose){
14
15 int i,filenum;
16 float x_cm, y_cm, u, v, lambda_nm, t_ns;
17 char cor_dir[60];
18 char stat_dir[60];
19 char cor_file[15];
20 char stat_file[15];
21
22 filenum=id;
23
24 // Event corsika file
25
26 //File labeling.
27
28 strcpy (cor_dir, "./");
29
30 sprintf(cor_file, "cer%06d",filenum);
31
32 strcat(cor_dir, cor_file);
33
34
35 // Fill the header of the corsika-like event.
36 //The fields in evt.fill are: event number, primary identifier, total energy (GeV),
37 // first target identifier, first z interaction(cm) , momentum x, momentum y, momentum z,
38 // zenith angle, azimuth angle, coreposition x (cm), coreposition y(cm)
39
40 ofstream cerfile;
41
42 if(!cerfile) {
43 cerr<<"Cannot create cerenkov file.\n";
44 exit(1);
45 }
46
47 cerfile.open(cor_dir, ios::out);
48
49 //____________________________________________________________________________________
50
51 cout<<"Writing binary Cherenkov file"<<" "<<cor_dir<<" "<<"..."<<endl;
52
53 cerevth.fill (1.0,
54 99.0, // primary id
55 inttime_s * 1e9, // instead of the total energy: integration time (ns)
56 1.0,
57 1.e7,
58 0.0,
59 0.0,
60 0.0,
61 0.0, // theta is always 0. !
62 0.0, // phi is always 0. !
63 0.0,
64 0.0);
65
66
67 cerevth.write(cerfile);
68
69
70 // Here we fill the information for each photon as a corsika particle.
71 // The fields in cerphot.fill are: wavelentgh (nm), x core position (cm), y core position (cm),
72 // u cosine director, v cosine director, time since first interaction (ns),
73 // height (cm) of first interaction.
74
75 for(i=0;i<photnum;i++){
76
77 lambda_nm = phot[i].lambda_nm;
78 x_cm = phot[i].x_m * 100.0;
79 y_cm = phot[i].y_m * 100.0;
80 u = phot[i].u;
81 v = phot[i].v;
82 t_ns = phot[i].arrtime_sec * 1e9;
83
84 cerphot.fill(lambda_nm,
85 x_cm,
86 y_cm,
87 u,
88 v,
89 t_ns,
90 1.e7);
91
92 cerphot.write(cerfile);
93 }
94
95 cerphot.fill(0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0);
96 cerphot.write(cerfile);
97
98 cerfile.close();
99
100 cout<<"Done."<<endl;
101
102 // Statistics corsika file
103
104 strcpy (stat_dir, "./");
105
106
107 //File labeling.
108
109 sprintf(stat_file, "sta%06d",filenum);
110
111 strcat(stat_dir, stat_file);
112
113 cerfile.open (stat_dir);
114
115 cout<<"Writing binary statistics file "<<" "<<stat_dir<<" "<<"..."<<endl;
116
117 cerstat.write(cerfile);
118
119 cerfile.close();
120
121 cout<<"Done."<<endl;
122
123 return 0;
124
125}
126
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