/* ======================================================================== *\ ! ! * ! * This file is part of CheObs, the Modular Analysis and Reconstruction ! * Software. It is distributed to you in the hope that it can be a useful ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes. ! * It is distributed WITHOUT ANY WARRANTY. ! * ! * Permission to use, copy, modify and distribute this software and its ! * documentation for any purpose is hereby granted without fee, ! * provided that the above copyright notice appears in all copies and ! * that both that copyright notice and this permission notice appear ! * in supporting documentation. It is provided "as is" without express ! * or implied warranty. ! * ! ! ! Author(s): Thomas Bretz, 1/2009 ! ! Copyright: CheObs Software Development, 2000-2010 ! ! \* ======================================================================== */ ////////////////////////////////////////////////////////////////////////////// // // MSimRays // // Task to produce rays from a light source at either infinity or a given // height from a given local sky position. // // The sky position is defined by an MPointingPos object in the parameter // list (if none exists, the source is at the reflector axis). Its // default name is "MPointingPos". // // The height of the light/point source is set by SetHeight in units of km. // A value <= 0 means infinity. // // The number of rays produced per event is defined by SetNumPhotons(n). // The default is 1000. // ////////////////////////////////////////////////////////////////////////////// #include "MSimRays.h" #include // root >=5.20 #include #include #include "MLog.h" #include "MLogManip.h" #include "MParList.h" #include "MQuaternion.h" #include "MPhotonEvent.h" #include "MPhotonData.h" #include "MOptics.h" #include "MPointingPos.h" ClassImp(MSimRays); using namespace std; // -------------------------------------------------------------------------- // // Default Constructor. // MSimRays::MSimRays(const char* name, const char *title) : fEvt(0), fReflector(0), fPointPos(0), fSource(0), fNumPhotons(1000), fHeight(-1), fWavelengthMin(-1), fWavelengthMax(-1), fNameReflector("MReflector"), fNamePointPos("MPointingPos"), fNameSource("Source") { fName = name ? name : "MSimRays"; fTitle = title ? title : "Task to calculate reflection os a mirror"; } // -------------------------------------------------------------------------- // // Search for the necessary parameter containers. // Int_t MSimRays::PreProcess(MParList *pList) { fEvt = (MPhotonEvent*)pList->FindCreateObj("MPhotonEvent"); if (!fEvt) return kFALSE; if (!pList->FindCreateObj("MCorsikaEvtHeader")) return kFALSE; fReflector = (MOptics*)pList->FindObject(fNameReflector, "MOptics"); if (!fReflector) { *fLog << inf << fNameReflector << " [MOptics] not found..." << endl; return kFALSE; } fSource = (MPointingPos*)pList->FindObject(fNameSource, "MPointingPos"); if (!fSource) { // *fLog << inf << fNameSource << " [MPointingPos] not found..." << endl; // return kFALSE; } fPointPos = (MPointingPos*)pList->FindObject(fNamePointPos, "MPointingPos"); if (!fPointPos) { *fLog << inf << fNamePointPos << " [MPointingPos] not found..." << endl; return kFALSE; } return kTRUE; } // -------------------------------------------------------------------------- // // Converts the photons into the telscope coordinate frame using the // pointing position from MPointingPos. // // Reflects all photons on all mirrors and stores the final photons on // the focal plane. Also intermediate photons are stored for debugging. // Int_t MSimRays::Process() { // Get arrays from event container fEvt->Resize(fNumPhotons); TClonesArray &arr = fEvt->GetArray(); const Int_t num = arr.GetEntriesFast(); const Double_t maxr = fReflector->GetMaxR(); const Double_t deltazd = fSource ? fSource->GetZdRad() : 0; const Double_t deltaaz = fSource ? fSource->GetAzRad() : 0; const Double_t zd = fPointPos->GetZdRad() + deltazd; const Double_t az = fPointPos->GetAzRad() + deltaaz; // cm -> m // s -> ns // length -> time const Double_t conv = 1./(TMath::C()*100/1e9); // Local sky coordinates (direction of telescope axis) //const Double_t zd = fPointing->GetZdRad(); // x==north //const Double_t az = fPointing->GetAzRad(); // Height of point source [cm] (0 means infinity) const Double_t h = fHeight * 100000; // Rotation matrix to derotate sky // For the new coordinate system see the Wiki TRotation rot; // The signs are positive because we align the incident point on ground to the telescope axis rot.RotateX( zd); // Rotate point on ground to align it with the telescope axis rot.RotateZ(-az); // tilt the point from ground to make it parallel to the mirror plane Int_t idx = 0; while (idx(arr.UncheckedAt(idx)); Double_t x, y; if (fHeight<0) { // Parallel light // -------------- const Double_t r = gRandom->Uniform(); gRandom->Circle(x, y, maxr*TMath::Sqrt(r)); } else { // Point source // ------------ // Adapted from: http://mathworld.wolfram.com/SpherePointPicking.html // Note that theta and phi is exchanged! // The maximum zenith angle is theta=atan(maxr/h) // cos(theta) = cos(atan(maxr/h)) = 1/sqrt(1+maxr^2/h^2) const double min_cost = 1./TMath::Sqrt(1.+maxr*maxr/h/h); const double cos_theta = gRandom->Uniform(min_cost, 1); gRandom->Circle(x, y, h*TMath::Sqrt(1./cos_theta/cos_theta - 1)); // const double cos_theta = gRandom->Uniform(ct, 1); // const double sin_theta = TMath::Sqrt(1.-cos_theta*cos_theta); // gRandom->Circle(x, y, h*sin_theta/cos_theta); // Homogeneous on a sphere // const double phi = TMath::TwoPi() * gRandom->Uniform(); // x = sin_theta * cos(phi); // y = sin_theta * sin(phi); // z = cos_theta; // Project the photons to a plane at z=1 // x /= cos_theta; // y /= cos_theta; // z /= cos_theta; // z = 1 // The radius of the sphere is h // x *= h; // y *= h; // z *= h; // z = h } // The is the incident direction of the photon // h==0 means infinitiy const TVector3 u = fHeight>0 ? TVector3(x, y, -h).Unit() : TVector3(0, 0, -1); // w is pointing away from the direction the photon comes from // CORSIKA-orig: x(north), y(west), z(up), t(time) // NOW: x(east), y(north), z(up), t(time) MQuaternion p(TVector3(x, y, 0), fHeight>0 ? TMath::Sqrt(x*x + y*y + h*h): 0); MQuaternion w(u, conv); // Rotate the coordinates into the reflector's coordinate system. // It is assumed that the z-plane is parallel to the focal plane. // (The reflector coordinate system is defined by the telescope orientation) p *= rot; w *= rot; // Now propagate the photon to the z-plane in the new coordinate system p.PropagateZ0(w); // Shift the coordinate system to the telescope. Corsika's // coordinate system is always w.r.t. to the particle axis //p += impact; // Store new position and direction in the reflector's coordinate frame dat.SetPosition(p); dat.SetDirection(w); if (fWavelengthMin>0 && fWavelengthMax>0) dat.SimWavelength(fWavelengthMin, fWavelengthMax); idx++; } // Doesn't seem to be too time consuming. But we could also sort later! // (after cones, inside the camera) // fEvt->Sort(kTRUE); return kTRUE; } // -------------------------------------------------------------------------- // // Height: -1 // NumPhotons: 1000 // Int_t MSimRays::ReadEnv(const TEnv &env, TString prefix, Bool_t print) { Bool_t rc = kFALSE; if (IsEnvDefined(env, prefix, "Height", print)) { rc = kTRUE; fHeight = GetEnvValue(env, prefix, "Height", fHeight); } if (IsEnvDefined(env, prefix, "NumPhotons", print)) { rc = kTRUE; fNumPhotons = GetEnvValue(env, prefix, "NumPhotons", (Int_t)fNumPhotons); } return rc; }