source: trunk/Mars/msim/MPhotonData.cc@ 19353

Last change on this file since 19353 was 19339, checked in by tbretz, 6 years ago
Added the 8-float format as FillEvtCorsikaThin, calculate absolute wavelength (right now, I don't know what to do with the information from the negative WL, print the origin only if it is defined, added some docu from the corsika docu, removed MMCS specific stuff by a pre-compiler directive -- do we still have MMCS data?
File size: 14.6 KB
Line 
1/* ======================================================================== *\
2!
3! *
4! * This file is part of CheObs, the Modular Analysis and Reconstruction
5! * Software. It is distributed to you in the hope that it can be a useful
6! * and timesaving tool in analysing Data of imaging Cerenkov telescopes.
7! * It is distributed WITHOUT ANY WARRANTY.
8! *
9! * Permission to use, copy, modify and distribute this software and its
10! * documentation for any purpose is hereby granted without fee,
11! * provided that the above copyright notice appears in all copies and
12! * that both that copyright notice and this permission notice appear
13! * in supporting documentation. It is provided "as is" without express
14! * or implied warranty.
15! *
16!
17!
18! Author(s): Thomas Bretz, 12/2000 <mailto:thomas.bretz@epfl.ch>
19! Author(s): Qi Zhe, 06/2007 <mailto:qizhe@astro.uni-wuerzburg.de>
20!
21! Copyright: CheObs Software Development, 2000-2010
22!
23!
24\* ======================================================================== */
25
26/////////////////////////////////////////////////////////////////////////////
27//
28// MPhotonData
29//
30// Storage container to store Corsika events
31//
32// For details on the coordinate systems see our Wiki.
33//
34// Version 1:
35// ----------
36// * First implementation
37//
38// Version 2:
39// ----------
40// - fNumPhotons
41//
42/////////////////////////////////////////////////////////////////////////////
43#include "MPhotonData.h"
44
45#include <fstream>
46#include <iostream>
47
48#include <TMath.h>
49#include <TRandom.h>
50
51#include "MLog.h"
52#include "MLogManip.h"
53
54ClassImp(MPhotonData);
55
56using namespace std;
57
58// --------------------------------------------------------------------------
59//
60// Default constructor.
61//
62MPhotonData::MPhotonData(/*const char *name, const char *title*/)
63 : fPosX(0), fPosY(0), fCosU(0), fCosV(0), fTime(0), fWavelength(0),
64 /*fNumPhotons(1),*/ fProductionHeight(0), fPrimary(MMcEvtBasic::kUNDEFINED),
65 fTag(-1), fMirrorTag(-1), fWeight(1)
66{
67 // fName = name ? name : "MPhotonData";
68 // fTitle = title ? title : "Corsika Event Data Information";
69}
70
71/*
72MPhotonData::MPhotonData(const MPhotonData &ph)
73: fPosX(ph.fPosX), fPosY(ph.fPosY), fCosU(ph.fCosU), fCosV(ph.fCosV),
74fTime(ph.fTime), fWavelength(ph.fWavelength), fNumPhotons(ph.fNumPhotons),
75fProductionHeight(ph.fProductionHeight), fPrimary(ph.fPrimary),
76fTag(ph.fTag), fWeight(ph.fWeight)
77{
78}
79*/
80
81// --------------------------------------------------------------------------
82//
83// Copy function. Copy all data members into obj.
84//
85void MPhotonData::Copy(TObject &obj) const
86{
87 MPhotonData &d = static_cast<MPhotonData&>(obj);
88
89// d.fNumPhotons = fNumPhotons;
90 d.fPosX = fPosX;
91 d.fPosY = fPosY;
92 d.fCosU = fCosU;
93 d.fCosV = fCosV;
94 d.fWavelength = fWavelength;
95 d.fPrimary = fPrimary;
96 d.fTime = fTime;
97 d.fTag = fTag;
98 d.fWeight = fWeight;
99 d.fProductionHeight = fProductionHeight;
100
101 TObject::Copy(obj);
102}
103
104// --------------------------------------------------------------------------
105//
106// Return the square cosine of the Theta-angle == 1-CosU^2-CosV^2
107//
108Double_t MPhotonData::GetCosW2() const
109{
110 return 1 - GetSinW2();
111}
112
113// --------------------------------------------------------------------------
114//
115// Return the square sine of the Theta-angle == CosU^2+CosV^2
116//
117Double_t MPhotonData::GetSinW2() const
118{
119 const Double_t sinw2 = fCosU*fCosU + fCosV*fCosV;
120 return sinw2>1 ? 1 : sinw2;
121}
122
123// --------------------------------------------------------------------------
124//
125// return the cosine of the Theta-angle == sqrt(1-CosU^2-CosV^2)
126//
127Double_t MPhotonData::GetCosW() const
128{
129 return TMath::Sqrt(GetCosW2());
130}
131
132// --------------------------------------------------------------------------
133//
134// return the sine of the Theta-angle == sqrt(CosU^2+CosV^2)
135//
136Double_t MPhotonData::GetSinW() const
137{
138 return TMath::Sqrt(GetSinW2());
139}
140
141// --------------------------------------------------------------------------
142//
143// Return the theta angle in radians
144//
145Double_t MPhotonData::GetTheta() const
146{
147 return TMath::ASin(GetSinW());
148}
149
150// --------------------------------------------------------------------------
151//
152// Return a TQuaternion with the first three components x, y, and z
153// and the fourth component the time.
154//
155TQuaternion MPhotonData::GetPosQ() const
156{
157 return TQuaternion(GetPos3(), fTime);
158}
159
160// --------------------------------------------------------------------------
161//
162// return a TQuaternion with the first three components the direction
163// moving in space (GetDir3()) and the fourth component is the
164// one devided by the speed of light (converted to cm/ns)
165//
166// FIXME: v in air!
167//
168TQuaternion MPhotonData::GetDirQ() const
169{
170 return TQuaternion(GetDir3(), 1./(TMath::C()*100/1e9));
171}
172
173// --------------------------------------------------------------------------
174//
175// Set the wavelength to a random lambda^-2 distributed value
176// between wmin and wmax.
177//
178void MPhotonData::SimWavelength(Float_t wmin, Float_t wmax)
179{
180 const Double_t w = gRandom->Uniform(wmin, wmax);
181
182 fWavelength = TMath::Nint(wmin*wmax / w);
183}
184
185
186// --------------------------------------------------------------------------
187//
188// Set the data member according to the 8 floats read from a reflector-file.
189// This function MUST reset all data-members, no matter whether these are
190// contained in the input stream.
191//
192Int_t MPhotonData::FillRfl(const Float_t f[8])
193{
194 // Check coordinate system!!!!
195 fWavelength = TMath::Nint(f[0]);
196 fPosX = f[1]; // [cm]
197 fPosY = f[2]; // [cm]
198 fCosU = f[3]; // cos to x
199 fCosV = f[4]; // cos to y
200 fTime = f[5]; // [ns]
201 fProductionHeight = f[6];
202
203 // f[7]: Camera inclination angle
204
205 fPrimary = MMcEvtBasic::kUNDEFINED;
206// fNumPhotons = 1;
207 fTag = -1;
208 fWeight = 1;
209
210 return kTRUE;
211}
212
213// --------------------------------------------------------------------------
214//
215// Set the data member according to the 7 floats read from a corsika-file.
216// This function MUST reset all data-members, no matter whether these are
217// contained in the input stream.
218//
219// Currently we exchange x and y and set y=-y to convert Corsikas coordinate
220// system intpo our own.
221//
222Int_t MPhotonData::FillCorsika(const Float_t f[7], Int_t i)
223{
224 // From the Corsika manual:
225 //
226 // f[0] : n Number of Cherenkov photons in bunch
227 // (For THIN option multiplied with thinning weight)
228 // f[1] : x [cm]
229 // f[2] : y [cm]
230 // f[3] : u direction cosine (to x axis) [u = sin(theta)cos(phi)]
231 // f[4] : v direction cosine (to y axis) [v = sin(theta)sin(phi)]
232 // f[5] : t [ns] time to first interaction or since start of atmosphere (see TSTART)
233 // f[6] : h [ch] bunch production height (except MCERFI=3)
234 // f[7] : w weight of bunch [only with THIN option]
235
236 // f[0] = MCERFI==1/2/3 && !THIN ? PHOTCM : PHOTCM*WTCER/MAX(1e-10, PROBTH)
237 // f[1] = XCER
238 // f[2] = YXCER
239 // f[3] = UEMIS
240 // f[4] = VEMIS
241 // f[5] = CARTIM
242 // f[6] = MCERFI<3 ? ZEMIS : CERDIST
243 // #if __THIN__
244 // f[7] = MCERFI==1 ? WTCER/MAX(1e-10, PROBTH) : (CEFFIC || CERWLEN ? WL*WLFLAG : WLFLAG);
245 // #endif
246 //
247 // WLFLAG = [CEFFIC=-1] [CERWLEN=1] [ELSE=0]
248 //
249 // WL = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*RDM(IRDM))
250 //
251 // WL-MIN = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*0) = WAVLGU
252 // WL-MAX = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*1) = WAVLGL
253 //
254
255 const UInt_t n /*fWeight*/ = TMath::Nint(f[0]);
256
257 // Empty bunch (this happend at the end of events when
258 // the remaining block is filled with zeroes)
259 if (f[0]==0)
260 return kCONTINUE;
261
262 if (f[0]!=1)
263 cout << "WARNING - Bunch size !=1 (" << f[0] << ")" <<endl;
264
265#ifdef __MMCS__
266 // Check reuse
267 if (i >=0)
268 {
269 const Int_t reuse = (n/1000)%100; // Force this to be 1!
270 if (reuse!=i)
271 {
272 cout << "REUSE " << reuse << " " << i << " " << n << endl;
273 return kCONTINUE;
274 }
275 }
276
277 // This seems to be special to mmcs
278 fWavelength = n%1000;
279 fPrimary = MMcEvtBasic::ParticleId_t(n/100000);
280#else
281 fWavelength = 0;
282 fPrimary = MMcEvtBasic::kUNDEFINED;
283#endif
284
285 // x=north, y=west
286 //fPosX = f[1]; // [cm]
287 //fPosY = f[2]; // [cm]
288 //fCosU = f[3]; // cos to x
289 //fCosV = f[4]; // cos to y
290 // x=west, y=south
291 fPosX = f[2]; // [cm]
292 fPosY = -f[1]; // [cm]
293
294 fCosU = f[4]; // cos to x
295 fCosV = -f[3]; // cos to y
296
297 fTime = f[5]; // [ns]
298
299 fProductionHeight = f[6]; // [cm]
300
301 // Now reset all data members which are not in the stream
302 fTag = -1;
303 fWeight = 1;
304
305 return kTRUE;
306}
307
308Int_t MPhotonData::FillCorsikaThin(const Float_t f[8], Int_t i)
309{
310 // From the Corsika manual:
311 //
312 // f[0] : n Number of Cherenkov photons in bunch
313 // (For THIN option multiplied with thinning weight)
314 // f[1] : x [cm]
315 // f[2] : y [cm]
316 // f[3] : u direction cosine (to x axis) [u = sin(theta)cos(phi)]
317 // f[4] : v direction cosine (to y axis) [v = sin(theta)sin(phi)]
318 // f[5] : t [ns] time to first interaction or since start of atmosphere (see TSTART)
319 // f[6] : h [ch] bunch production height (except MCERFI=3)
320 // f[7] : w weight of bunch [only with THIN option]
321
322 // f[0] = MCERFI==1/2/3 && !THIN ? PHOTCM : PHOTCM*WTCER/MAX(1e-10, PROBTH)
323 // f[1] = XCER
324 // f[2] = YXCER
325 // f[3] = UEMIS
326 // f[4] = VEMIS
327 // f[5] = CARTIM
328 // f[6] = MCERFI<3 ? ZEMIS : CERDIST
329 // #if __THIN__
330 // f[7] = MCERFI==1 ? WTCER/MAX(1e-10, PROBTH) : (CEFFIC || CERWLEN ? WL*WLFLAG : WLFLAG);
331 // #endif
332 //
333 // WLFLAG = [CEFFIC=-1] [CERWLEN=1] [ELSE=0]
334 //
335 // WL = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*RDM(IRDM))
336 //
337 // WL-MIN = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*0) = WAVLGU
338 // WL-MAX = 1./(1./WAVLGU+(1./WAVLGL-1./WAVLGU)*1) = WAVLGL
339 //
340
341 const UInt_t n /*fWeight*/ = TMath::Nint(f[0]);
342
343 // Empty bunch (this happend at the end of events when
344 // the remaining block is filled with zeroes)
345 if (f[0]==0)
346 return kCONTINUE;
347
348 if (f[0]!=1)
349 cout << "WARNING - Bunch size !=1 (" << f[0] << ")" <<endl;
350
351
352 // x=north, y=west
353 //fPosX = f[1]; // [cm]
354 //fPosY = f[2]; // [cm]
355 //fCosU = f[3]; // cos to x
356 //fCosV = f[4]; // cos to y
357 // x=west, y=south
358 fPosX = f[2]; // [cm]
359 fPosY = -f[1]; // [cm]
360
361 fCosU = f[4]; // cos to x
362 fCosV = -f[3]; // cos to y
363
364 fTime = f[5]; // [ns]
365
366 fProductionHeight = f[6]; // [cm]
367
368 fWavelength = TMath::Abs(f[7]);
369
370 // Now reset all data members which are not in the stream
371 fPrimary = MMcEvtBasic::kUNDEFINED;
372 fTag = -1;
373 fWeight = 1;
374
375 return kTRUE;
376}
377
378// --------------------------------------------------------------------------
379//
380// Set the data member according to the 8 shorts read from a eventio-file.
381// This function MUST reset all data-members, no matter whether these are
382// contained in the input stream.
383//
384// Currently we exchange x and y and set y=-y to convert Corsikas coordinate
385// system into our own.
386//
387Int_t MPhotonData::FillEventIO(const Short_t f[8])
388{
389 // From 5.5 compact_bunch:
390 // https://www.mpi-hd.mpg.de/hfm/~bernlohr/iact-atmo/iact_refman.pdf
391
392 // photons in this bunch f[6]/100.
393
394 fPosY = -f[0]/10.; // ypos relative to telescope [cm]
395 fPosX = f[1]/10.; // xpos relative to telescope [cm]
396 fCosV = -f[2]/30000.; // cos to y
397 fCosU = f[3]/30000.; // cos to x
398
399 fTime = f[4]/10.; // a relative arival time [ns]
400 fProductionHeight = pow(10, f[5]/1000.); // altitude of emission a.s.l. [cm]
401 fWavelength = TMath::Abs(f[7]); // wavelength [nm]: 0 undetermined, <0 already in p.e.
402
403 // Now reset all data members which are not in the stream
404 fPrimary = MMcEvtBasic::kUNDEFINED;
405 fTag = -1;
406 fWeight = 1;
407
408 return 1;
409}
410
411// --------------------------------------------------------------------------
412//
413// Set the data member according to the 8 floats read from a eventio-file.
414// This function MUST reset all data-members, no matter whether these are
415// contained in the input stream.
416//
417// Currently we exchange x and y and set y=-y to convert Corsikas coordinate
418// system into our own.
419//
420Int_t MPhotonData::FillEventIO(const Float_t f[8])
421{
422 // photons in this bunch
423 const UInt_t n = TMath::Nint(f[6]);
424 if (n==0)
425 return 0;
426
427 fPosX = f[1]; // xpos relative to telescope [cm]
428 fPosY = -f[0]; // ypos relative to telescope [cm]
429 fCosU = f[3]; // cos to x
430 fCosV = -f[2]; // cos to y
431 //fTime = f[4]; // a relative arival time [ns]
432 //fProductionHeight = f[5]; // altitude of emission [cm]
433 fWavelength = 0; // so far always zeor = unspec. [nm]
434
435 // Now reset all data members which are not in the stream
436 fPrimary = MMcEvtBasic::kUNDEFINED;
437 fTag = -1;
438 fWeight = 1;
439
440 return n-1;
441}
442
443/*
444// --------------------------------------------------------------------------
445//
446// Read seven floats from the stream and call FillCorsika for them.
447//
448Int_t MPhotonData::ReadCorsikaEvt(istream &fin)
449{
450 Float_t f[7];
451 fin.read((char*)&f, 7*4);
452
453 const Int_t rc = FillCorsika(f);
454
455 return rc==kTRUE ? !fin.eof() : rc;
456}
457
458// --------------------------------------------------------------------------
459//
460// Read eight floats from the stream and call FillRfl for them.
461//
462Int_t MPhotonData::ReadRflEvt(istream &fin)
463{
464 Float_t f[8];
465 fin.read((char*)&f, 8*4);
466
467 const Int_t rc = FillRfl(f);
468
469 return rc==kTRUE ? !fin.eof() : rc;
470}
471*/
472
473// --------------------------------------------------------------------------
474//
475// Print contents. The tag and Weight are only printed if they are different
476// from the default.
477//
478void MPhotonData::Print(Option_t *) const
479{
480 gLog << inf << endl;
481 // gLog << "Num Photons: " << fNumPhotons << " from " << MMcEvtBasic::GetParticleName(fPrimary) << endl;
482 if (fPrimary!=MMcEvtBasic::kUNDEFINED)
483 gLog << "Origin: " << MMcEvtBasic::GetParticleName(fPrimary) << endl;
484 gLog << "Wavelength: " << fWavelength << "nm" << endl;
485 gLog << "Pos X/Y Cos U/V: " << fPosX << "/" << fPosY << " " << fCosU << "/" << fCosV << endl;
486 gLog << "Time/Prod.Height: " << fTime << "ns/" << fProductionHeight/100 << "m" << endl;
487 if (fTag>=0)
488 gLog << "Tag: " << fTag << endl;
489 if (fWeight!=1)
490 gLog << "Weight: " << fWeight << endl;
491}
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