| 1 | /* ======================================================================== *\
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| 2 | !
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| 3 | ! *
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| 4 | ! * This file is part of MARS, the MAGIC Analysis and Reconstruction
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| 5 | ! * Software. It is distributed to you in the hope that it can be a useful
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| 6 | ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes.
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| 7 | ! * It is distributed WITHOUT ANY WARRANTY.
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| 8 | ! *
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| 9 | ! * Permission to use, copy, modify and distribute this software and its
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| 10 | ! * documentation for any purpose is hereby granted without fee,
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| 11 | ! * provided that the above copyright notice appear in all copies and
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| 12 | ! * that both that copyright notice and this permission notice appear
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| 13 | ! * in supporting documentation. It is provided "as is" without express
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| 14 | ! * or implied warranty.
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| 15 | ! *
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| 16 | !
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| 17 | !
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| 18 | ! Author(s): Thomas Bretz 12/2000 <mailto:tbretz@astro.uni-wuerzburg.de>
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| 19 | Qi Zhe, 06/2007 <mailto:qizhe@astro.uni-wuerzburg.de>
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| 20 |
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| 21 | ! Copyright: Software Development, 2000-2009
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| 22 | !
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| 23 | !
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| 24 | \* ======================================================================== */
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| 25 |
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| 26 | /////////////////////////////////////////////////////////////////////////////
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| 27 | //
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| 28 | // MCorsikaRunHeader
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| 29 | //
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| 30 | // Root storage container for the RUN HEADER information
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| 31 | //
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| 32 | // Class Version 2:
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| 33 | // ----------------
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| 34 | // + UInt_t fParticleID
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| 35 | // + Float_t fImpactMax
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| 36 | // + Float_t fMagneticFieldX
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| 37 | // + Float_t fMagneticFieldZ
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| 38 | // + Float_t fMagneticFieldAz
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| 39 | // + Float_t fAtmosphericLayers[5]
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| 40 | // + Float_t fAtmosphericCoeffA[5]
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| 41 | // + Float_t fAtmosphericCoeffB[5]
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| 42 | // + Float_t fAtmosphericCoeffC[5]
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| 43 | // + UInt_t fCerenkovFlag
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| 44 | //
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| 45 | // Class Version 3:
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| 46 | // ----------------
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| 47 | // + UInt_t fNumReuse
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| 48 | //
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| 49 | // Class Version 4:
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| 50 | // ----------------
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| 51 | // + UInt_t fCerenkovFileOption
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| 52 | // + UInt_t fHadronModelLowEnergy
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| 53 | // + UInt_t fHadronModelHighEnergy
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| 54 | // + Float_t fTransitionEnergy
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| 55 | // + Bool_t fCurvedAtmosphere
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| 56 | // + Float_t fEnergyCutoffHadrons
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| 57 | // + Float_t fEnergyCutoffMuons
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| 58 | // + Float_t fEnergyCutoffElectrons
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| 59 | // + Float_t fEnergyCutoffPhotons
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| 60 | // + Float_t fThinningEnergyFractionH
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| 61 | // + Float_t fThinningEnergyFractionEM
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| 62 | // + Float_t fThinningWeightLimitH
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| 63 | // + Float_t fThinningWeightLimitEM
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| 64 | // + Float_t fThinningMaxRadius
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| 65 | //
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| 66 | ////////////////////////////////////////////////////////////////////////////
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| 67 |
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| 68 | #include "MCorsikaRunHeader.h"
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| 69 | #include "MCorsikaFormat.h"
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| 70 |
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| 71 | #include <fstream>
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| 72 | #include <iomanip>
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| 73 |
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| 74 | #include "MLog.h"
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| 75 | #include "MLogManip.h"
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| 76 |
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| 77 | #include "MMcEvt.hxx"
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| 78 |
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| 79 | ClassImp(MCorsikaRunHeader);
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| 80 |
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| 81 | using namespace std;
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| 82 |
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| 83 | const Double_t MCorsikaRunHeader::fgEarthRadius = 637131500; // [cm] Earth radius as defined in CORSIKA
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| 84 |
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| 85 | // --------------------------------------------------------------------------
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| 86 | //
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| 87 | // Default constructor. Creates array which stores the pixel assignment.
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| 88 | //
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| 89 | //
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| 90 | MCorsikaRunHeader::MCorsikaRunHeader(const char *name, const char *title)
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| 91 | : fNumObsLevel(0), fImpactMax(-1), fZdMin(0), fZdMax(-1),
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| 92 | fAzMin(0), fAzMax(0), fWavelengthMin(-1), fWavelengthMax(-1),
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| 93 | fViewConeInnerAngle(0), fViewConeOuterAngle(-1)
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| 94 | {
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| 95 | fName = name ? name : "MCorsikaRunHeader";
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| 96 | fTitle = title ? title : "Raw Run Header Information";
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| 97 | }
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| 98 |
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| 99 | // --------------------------------------------------------------------------
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| 100 | //
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| 101 | // Read in one run header from the binary file
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| 102 | //
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| 103 | Bool_t MCorsikaRunHeader::ReadEvt(MCorsikaFormat * fInFormat, const uint32_t &blockLength)
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| 104 | {
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| 105 | vector<Float_t> f(blockLength);
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| 106 | if (!fInFormat->Read(f.data(), blockLength*sizeof(Float_t)))
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| 107 | return kFALSE;
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| 108 |
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| 109 | fRunNumber = TMath::Nint(f[0]);
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| 110 | fNumEvents = 0;
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| 111 |
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| 112 | fRunStart.SetCorsikaTime(f[1]);
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| 113 |
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| 114 | fProgramVersion = f[2];
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| 115 | fNumObsLevel = TMath::Nint(f[3]);
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| 116 |
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| 117 | if (fNumObsLevel!=1)
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| 118 | {
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| 119 | *fLog << err << "ERROR - Currently only one observation level is allowed." << endl;
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| 120 | return kFALSE;
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| 121 | }
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| 122 |
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| 123 | memset(fObsLevel, 0, 10*4);
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| 124 | memcpy(fObsLevel, f.data()+4, fNumObsLevel*4);
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| 125 |
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| 126 | fSlopeSpectrum = f[14];
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| 127 | fEnergyMin = f[15];
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| 128 | fEnergyMax = f[16];
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| 129 |
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| 130 | fEnergyCutoffHadrons = f[17];
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| 131 | fEnergyCutoffMuons = f[18];
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| 132 | fEnergyCutoffElectrons = f[19];
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| 133 | fEnergyCutoffPhotons = f[20];
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| 134 |
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| 135 | // Implemented in CORSIKA Version >= 6.822
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| 136 | fImpactMax = -1;
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| 137 |
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| 138 | // CORSIKA scattering in a disc on the ground
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| 139 | if (f[246]>0 && f[247]==0 && !fInFormat->IsEventioFormat())
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| 140 | {
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| 141 | *fLog << warn << "WARNING - Events scattered in a disc on the ground." << endl;
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| 142 | fImpactMax = f[246];
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| 143 | }
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| 144 |
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| 145 | // MMCS scattering in a disc perpendicular to the shower axis
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| 146 | if (f[246]==0 && f[247]>0)
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| 147 | fImpactMax = f[247];
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| 148 |
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| 149 | // CORSIKA scattering in a rectangle on the ground
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| 150 | if (f[246]>0 && f[247]>0)
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| 151 | *fLog << warn << "WARNING - Events scattered in a rectangle on the ground." << endl;
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| 152 |
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| 153 | // Implemented in CORSIKA Version >= 6.822
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| 154 | memcpy(fAtmosphericLayers, f.data()+248, 5*4);
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| 155 |
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| 156 | memcpy(fAtmosphericCoeffA, f.data()+253, 5*4);
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| 157 | memcpy(fAtmosphericCoeffB, f.data()+258, 5*4);
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| 158 | memcpy(fAtmosphericCoeffC, f.data()+263, 5*4);
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| 159 |
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| 160 | return kTRUE;
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| 161 | }
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| 162 |
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| 163 | // --------------------------------------------------------------------------
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| 164 | //
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| 165 | // Read in one event header. It is called for the first event header after
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| 166 | // a run header
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| 167 | //
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| 168 | Bool_t MCorsikaRunHeader::ReadEventHeader(Float_t * g)
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| 169 | {
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| 170 |
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| 171 | // -------------------- Read first event header -------------------
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| 172 |
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| 173 | // FIXME: Add sanity checks!
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| 174 |
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| 175 | // f[76] Cherenkov flag:
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| 176 | // bit(1) : CERENKOV option compiled in
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| 177 | // bit(2) : IACT option compiled in
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| 178 | // bit(3) : CEFFIC option compiled in
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| 179 | // bit(4) : ATMEXT option compiled in
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| 180 | // bit(5) : ATMEXT option used with refraction enabled
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| 181 | // bit(6) : VOLUMEDET option compiled in
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| 182 | // bit(7) : CURVED option compiled in
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| 183 | // bit(9) : SLATN option compiled in
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| 184 | // 11-21 : table number for externam athmosphere (but<1024)
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| 185 | //
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| 186 | // f[78] Curved athmosphere? (0=flat, 1=curved)
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| 187 | // f[84] cherenkov bunch size
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| 188 | // f[93] flag for additinal muon information of particle output file
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| 189 | // f[145] Muon multiple scattering flag
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| 190 |
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| 191 |
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| 192 | fNumReuse = TMath::Nint(g[96]); // Number i of uses of each cherenkov event
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| 193 |
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| 194 | fParticleID = TMath::Nint(g[1]);
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| 195 |
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| 196 | // MAGNETIC FIELD: x/z-component of earth magnetic field in muT
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| 197 | fMagneticFieldX = g[69]; // x-component ( BX)
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| 198 | fMagneticFieldZ = -g[70]; // z-component (-BZ)
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| 199 | fMagneticFieldAz = g[91]; // Azimuth angle of magnetic north expressed in telescope coordinates
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| 200 |
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| 201 | fHadronModelLowEnergy = TMath::Nint(g[73]);
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| 202 | fHadronModelHighEnergy = TMath::Nint(g[74]);
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| 203 |
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| 204 | // WITH rounding: unbelievable!
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| 205 | fCerenkovFlag = TMath::Nint(g[75]);
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| 206 | fCerenkovFileOption = TMath::Nint(g[90]);
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| 207 |
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| 208 | fCurvedAtmosphere = TMath::Nint(g[77])==2;
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| 209 |
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| 210 | fZdMin = g[79]; // lower edge of theta in °
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| 211 | fZdMax = g[80]; // upper edge of theta in °
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| 212 | fAzMin = 180-g[81]; // lower edge of phi in °
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| 213 | fAzMax = 180-g[82]; // upper edge of phi in °
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| 214 | // FIXME: Correct for direction of magnetic field!
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| 215 |
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| 216 | if (TMath::Nint(g[83])!=1)
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| 217 | *fLog << warn << "WARNING - Cherenkov bunch size not 1, but " << g[83] << endl;
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| 218 |
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| 219 | // g[84] Number of cherenkov detectors in x
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| 220 | // g[85] Number of cherenkov detectors in y
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| 221 | // g[86] Grid spacing x
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| 222 | // g[87] Grid spacing y
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| 223 | // g[88] Length of detectors in x
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| 224 | // g[89] Length of detectors in y
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| 225 |
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| 226 | fImpactMax = -1;
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| 227 | /*
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| 228 | // This is a trick to use CERARY for storage of the
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| 229 | // maximum simulated impact
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| 230 | if (TMath::Nint(g[84])==1 && TMath::Nint(g[85])==1 &&
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| 231 | TMath::Nint(g[88])==1 && TMath::Nint(g[89])==1 &&
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| 232 | g[86]==g[87])
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| 233 | fImpactMax = g[86];
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| 234 | */
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| 235 | fWavelengthMin = g[94]; // Cherenkov bandwidth lower end in nm
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| 236 | fWavelengthMax = g[95]; // Cherenkov bandwidth upper end in nm
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| 237 |
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| 238 | fThinningEnergyFractionH = g[146]; // EFRCTHN
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| 239 | fThinningEnergyFractionEM = g[147]; // EFRCTHN*THINRAT
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| 240 | fThinningWeightLimitH = g[148]; // WMAX
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| 241 | fThinningWeightLimitEM = g[149]; // WMAX*WEITRAT
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| 242 | fThinningMaxRadius = g[150]; // Max radial radius for thinning
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| 243 |
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| 244 | fViewConeInnerAngle = g[151]; // inner angle of view cone (°)
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| 245 | fViewConeOuterAngle = g[152]; // outer angle of view cone (°)
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| 246 |
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| 247 | fTransitionEnergy = g[153];
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| 248 |
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| 249 | return kTRUE;
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| 250 | }
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| 251 |
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| 252 | Bool_t MCorsikaRunHeader::ReadEvtEnd(MCorsikaFormat * fInFormat, Bool_t runNumberVerify)
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| 253 | {
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| 254 | Float_t f[2];
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| 255 | if (!fInFormat->Read(f, 2 * sizeof(Float_t)))
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| 256 | return kFALSE;
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| 257 |
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| 258 | if (runNumberVerify)
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| 259 | {
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| 260 | const UInt_t runnum = TMath::Nint(f[0]);
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| 261 | if (runnum!=fRunNumber)
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| 262 | {
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| 263 | *fLog << err << "ERROR - Mismatch in stream: Run number in RUNE (";
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| 264 | *fLog << runnum << ") doesn't match RUNH (" << fRunNumber << ")." << endl;
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| 265 | return kFALSE;
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| 266 | }
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| 267 | }
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| 268 |
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| 269 | fNumEvents = TMath::Nint(f[1]);
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| 270 |
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| 271 | return kTRUE;
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| 272 | }
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| 273 |
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| 274 | // --------------------------------------------------------------------------
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| 275 | //
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| 276 | // print run header information on *fLog. The option 'header' supresses
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| 277 | // the pixel index translation table.
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| 278 | //
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| 279 | void MCorsikaRunHeader::Print(Option_t *t) const
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| 280 | {
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| 281 | *fLog << all << endl;
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| 282 | *fLog << "Run Number: " << fRunNumber << " (" << fRunStart.GetStringFmt("%d.%m.%Y") << ", V" << fProgramVersion << ")" << endl;
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| 283 | *fLog << "Particle ID: " << MMcEvt::GetParticleName(fParticleID) << endl;
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| 284 | if (fNumEvents>0)
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| 285 | *fLog << "Num Events: " << fNumEvents << " (reuse " << fNumReuse << " times)" << endl;
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| 286 | *fLog << "Obs Level: ";
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| 287 | for (Byte_t i=0; i<fNumObsLevel; i++)
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| 288 | *fLog << " " << fObsLevel[i]/100. << "m";
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| 289 | *fLog << endl;
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| 290 |
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| 291 | *fLog << "MagneticField: X/Z=(" << fMagneticFieldX << "/";
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| 292 | *fLog << fMagneticFieldZ << ")" << UTF8::kMu << "T Az=" << fMagneticFieldAz*TMath::RadToDeg() << UTF8::kDeg << " (magnetic North w.r.t. North)" << endl;
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| 293 |
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| 294 | *fLog << "Spectrum: Slope=" << fSlopeSpectrum << " (" << fEnergyMin << "GeV-" << fEnergyMax << "GeV)" << endl;
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| 295 | *fLog << "Wavelength: " << fWavelengthMin << "nm - " << fWavelengthMax << "nm" << endl;
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| 296 |
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| 297 | if (fImpactMax>0)
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| 298 | *fLog << "ImpactMax: " << fImpactMax << "cm" << endl;
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| 299 | if (fViewConeOuterAngle>0)
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| 300 | *fLog << "ViewCone: " << fViewConeInnerAngle << UTF8::kDeg << " - " << fViewConeOuterAngle << UTF8::kDeg << endl;
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| 301 |
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| 302 | *fLog << "Zd/Az: ";
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| 303 | if (fZdMax>=0 && fZdMin<360)
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| 304 | {
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| 305 | *fLog << fZdMin << UTF8::kDeg;
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| 306 | if (fZdMin==fZdMax)
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| 307 | *fLog << " (fixed)";
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| 308 | else
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| 309 | *fLog << "-" << fZdMax << UTF8::kDeg;
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| 310 | *fLog << " / " << fAzMin << UTF8::kDeg;
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| 311 | if (fAzMin==fAzMax)
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| 312 | *fLog << " (fixed)";
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| 313 | else
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| 314 | *fLog << "-" << fAzMax << UTF8::kDeg;
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| 315 | *fLog << " w.r.t. magnetic North." << endl;
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| 316 | }
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| 317 |
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| 318 | if (fZdMin>=360) // 4010.7
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| 319 | *fLog << "-trajectory-" << endl;
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| 320 |
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| 321 |
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| 322 | if (fImpactMax>0)
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| 323 | *fLog << "Max.sim.Impact: " << fImpactMax << "cm" << endl;
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| 324 |
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| 325 | *fLog << "Energy cutoff: ";
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| 326 | *fLog << fEnergyCutoffHadrons << "GeV (hadrons), ";
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| 327 | *fLog << fEnergyCutoffMuons << "GeV (muons), ";
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| 328 | *fLog << fEnergyCutoffElectrons << "GeV (electrons), ";
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| 329 | *fLog << fEnergyCutoffPhotons << "GeV (photons)";
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| 330 | *fLog << endl;
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| 331 |
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| 332 | *fLog << "Thinning: ";
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| 333 | if (fThinningWeightLimitH>0)
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| 334 | {
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| 335 | *fLog << "HADRONIC: E/Eth>" << fThinningEnergyFractionH << " (w>" << fThinningWeightLimitH << "), ";
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| 336 | *fLog << "EM: E/Eth>" << fThinningEnergyFractionEM << " (w>" << fThinningWeightLimitEM << "), ";
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| 337 | *fLog << "R>" << fThinningMaxRadius << "cm";
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| 338 | *fLog << endl;
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| 339 | }
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| 340 | else
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| 341 | *fLog << "<off>" << endl;
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| 342 |
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| 343 | *fLog << "Interact.model: ";
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| 344 | switch (fHadronModelLowEnergy)
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| 345 | {
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| 346 | case 1: *fLog << "GEISHA"; break;
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| 347 | case 2: *fLog << "UrQMD"; break;
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| 348 | case 3: *fLog << "FLUKA"; break;
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| 349 | default: *fLog << "<n/a>"; break;
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| 350 | }
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| 351 | *fLog << " / ";
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| 352 | switch (fHadronModelHighEnergy)
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| 353 | {
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| 354 | case 0: *fLog << "HDPM"; break;
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| 355 | case 1: *fLog << "VENUS"; break;
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| 356 | case 2: *fLog << "SIBYLL"; break;
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| 357 | case 3: *fLog << "QGSJET"; break;
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| 358 | case 4: *fLog << "DPMJET"; break;
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| 359 | case 5: *fLog << "neXus"; break;
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| 360 | case 6: *fLog << "EPOS"; break;
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| 361 | default: *fLog << "<n/a>"; break;
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| 362 | }
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| 363 | *fLog << " [lo/hi], Transition at " << fTransitionEnergy << " GeV" << endl;
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| 364 |
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| 365 | *fLog << "Options used: ";
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| 366 | if (Has(kCerenkov))
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| 367 | *fLog << " CERENKOV";
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| 368 | if (Has(kIact))
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| 369 | *fLog << " IACT";
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| 370 | if (Has(kCeffic))
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| 371 | *fLog << " CEFFIC";
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| 372 | if (Has(kAtmext))
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| 373 | *fLog << " ATMEXT" << GetNumAtmosphericModel();
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| 374 | if (Has(kRefraction))
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| 375 | *fLog << " +Refraction";
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| 376 | if (Has(kVolumedet))
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| 377 | *fLog << " VOLUMEDET";
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| 378 | if (Has(kCurved))
|
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| 379 | *fLog << " CURVED" << (fCurvedAtmosphere?"<on>":"<off>");
|
|---|
| 380 | if (Has(kSlant))
|
|---|
| 381 | *fLog << " SLANT";
|
|---|
| 382 | *fLog << " [" << hex << fCerenkovFlag << "]" << dec << endl;
|
|---|
| 383 |
|
|---|
| 384 | if (Has(kCerenkov))
|
|---|
| 385 | {
|
|---|
| 386 | *fLog << "File format: ";
|
|---|
| 387 | switch (fCerenkovFileOption)
|
|---|
| 388 | {
|
|---|
| 389 | case 0:
|
|---|
| 390 | *fLog << "Cerenkov photons written to DAT-file.";
|
|---|
| 391 | break;
|
|---|
| 392 | case 1:
|
|---|
| 393 | *fLog << "Cerenkov photons written to CER-file";
|
|---|
| 394 | break;
|
|---|
| 395 | case 2:
|
|---|
| 396 | *fLog << "Cerenkov photons written to CER-file / Wavelength as 8th item in THIN option";
|
|---|
| 397 | break;
|
|---|
| 398 | default:
|
|---|
| 399 | *fLog << "Cerenkov photons written to CER-file / Prod. height replaced by distance to array center.";
|
|---|
| 400 | break;
|
|---|
| 401 | }
|
|---|
| 402 | *fLog << " [MCERFI=" << fCerenkovFileOption << "]" << endl;
|
|---|
| 403 | }
|
|---|
| 404 |
|
|---|
| 405 | if (HasLayers())
|
|---|
| 406 | {
|
|---|
| 407 | *fLog << "Atm.Layers: ";
|
|---|
| 408 | for (int i=0; i<5; i++)
|
|---|
| 409 | *fLog << " " << fAtmosphericLayers[i];
|
|---|
| 410 | }
|
|---|
| 411 | *fLog << endl;
|
|---|
| 412 | *fLog << "Atm.Coeff A: ";
|
|---|
| 413 | for (int i=0; i<5; i++)
|
|---|
| 414 | *fLog << " " << fAtmosphericCoeffA[i];
|
|---|
| 415 | *fLog << endl;
|
|---|
| 416 | *fLog << "Atm.Coeff B: ";
|
|---|
| 417 | for (int i=0; i<5; i++)
|
|---|
| 418 | *fLog << " " << fAtmosphericCoeffB[i];
|
|---|
| 419 | *fLog << endl;
|
|---|
| 420 | *fLog << "Atm.Coeff C: ";
|
|---|
| 421 | for (int i=0; i<5; i++)
|
|---|
| 422 | *fLog << " " << fAtmosphericCoeffC[i];
|
|---|
| 423 | *fLog << endl;
|
|---|
| 424 |
|
|---|
| 425 |
|
|---|
| 426 | }
|
|---|
| 427 |
|
|---|