| [601] | 1 | //-------------------------------------------------------------------------- | 
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|  | 2 | // File and Version Information: | 
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| [2144] | 3 | //      $Id: blackbody.cc,v 1.7 2002-07-31 10:25:34 ansari Exp $ | 
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| [601] | 4 | // | 
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|  | 5 | // Description: | 
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|  | 6 | //      Aim of the class: To give the energy density for a blackbody | 
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|  | 7 | //                        The unity used here is W/m^2/Hz/sr | 
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|  | 8 | // | 
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|  | 9 | // History (add to end): | 
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|  | 10 | //      Sophie   Oct, 1999  - creation | 
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|  | 11 | // | 
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|  | 12 | //------------------------------------------------------------------------ | 
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|  | 13 |  | 
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|  | 14 | //--------------- | 
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|  | 15 | // C++ Headers -- | 
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|  | 16 | //--------------- | 
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|  | 17 | #include "machdefs.h" | 
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|  | 18 | #include <iostream.h> | 
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|  | 19 | #include <math.h> | 
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|  | 20 | #include "blackbody.h" | 
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|  | 21 |  | 
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| [909] | 22 | /*! | 
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| [927] | 23 | * \class SOPHYA::BlackBody | 
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|  | 24 | \ingroup SkyT | 
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| [909] | 25 | This class corresponds to the emission spectrum of a | 
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|  | 26 | blackbody radiation. | 
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|  | 27 | */ | 
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| [601] | 28 | //---------------- | 
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|  | 29 | // Constructor -- | 
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|  | 30 | //---------------- | 
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| [909] | 31 | /*! Constructor: needs a temperature. Otherwise set to ConvTools::tcmb */ | 
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| [601] | 32 | BlackBody::BlackBody(double temperature) | 
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| [668] | 33 | : RadSpectra(10., 10000.) | 
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| [601] | 34 | { | 
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|  | 35 | _temperature = temperature; | 
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|  | 36 | } | 
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|  | 37 |  | 
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|  | 38 |  | 
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|  | 39 | BlackBody::~BlackBody() | 
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|  | 40 | { | 
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|  | 41 | } | 
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| [909] | 42 | /*! Black Body Flux Function: | 
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|  | 43 | \f[ | 
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|  | 44 | I_\nu = {2 h_{pl} (1.10^9*\nu)^3 \over c^2 (e^{{h_{pl}(1.10^9*\nu) \over kT}} -1)} | 
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|  | 45 | \f] | 
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|  | 46 | */ | 
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| [601] | 47 | double | 
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|  | 48 | BlackBody::flux(double nu) const | 
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|  | 49 | { | 
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|  | 50 | if(nu < -1.e99) nu = -1.e99; | 
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|  | 51 | if(nu > 1.e99) nu = 1.e99; | 
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|  | 52 | double temperature = getTemperature(); | 
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|  | 53 | if(nu==0.) return 0.; | 
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|  | 54 | double hpl = ConvTools::hpl; | 
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|  | 55 | double cel = ConvTools::cel; | 
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|  | 56 | double kb  = ConvTools::kb; | 
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| [2144] | 57 | double puiss1 = nu*pow(10.,9); | 
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| [601] | 58 | if(puiss1 >  1.e99)   puiss1=1.e99; | 
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|  | 59 | if(puiss1 < -1.e99)   puiss1=-1.e99; | 
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| [2144] | 60 | double puiss2 = hpl*nu*pow(10.,9)/(kb*temperature); | 
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| [601] | 61 | if(puiss2 >  1.e99)   puiss2=1.e99; | 
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|  | 62 | if(puiss2 < -1.e99)   puiss2=-1.e99; | 
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|  | 63 |  | 
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|  | 64 | double result= | 
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|  | 65 | (2*hpl* pow( puiss1 ,3))/( pow(cel,2)*(exp(puiss2)-1)); | 
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|  | 66 | return result; | 
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|  | 67 | } | 
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|  | 68 |  | 
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| [669] | 69 |  | 
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|  | 70 | void | 
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|  | 71 | BlackBody::Print(ostream& os) const | 
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|  | 72 | { | 
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|  | 73 | os << "BlackBody::Print Temp= " << getTemperature() | 
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|  | 74 | << " - Fmin,Fmax= " << minFreq() << "," << maxFreq() << endl; | 
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|  | 75 | os << "MeanFreq= " << meanFreq() << "  Emission= " << flux(meanFreq()) << endl; | 
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|  | 76 | os << "PeakFreq= " << peakFreq() << "  Emission= " << flux(peakFreq()) << endl; | 
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|  | 77 |  | 
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|  | 78 | } | 
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|  | 79 |  | 
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|  | 80 | /* | 
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| [668] | 81 | void | 
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|  | 82 | BlackBody::WriteSelf(POutPersist& s) | 
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|  | 83 | { | 
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|  | 84 | s.PutR8(this->getTemperature()); | 
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|  | 85 | s.PutR8(this->minFreq()); | 
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|  | 86 | s.PutR8(this->maxFreq()); | 
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|  | 87 | } | 
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|  | 88 |  | 
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| [601] | 89 | void | 
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| [668] | 90 | BlackBody::ReadSelf(PInPersist& s) | 
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|  | 91 | { | 
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|  | 92 | s.GetR8(_temperature); | 
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|  | 93 | s.GetR8(_numin); | 
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|  | 94 | s.GetR8(_numax); | 
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|  | 95 | cout << " Temperature - minFreq - maxFreq " << endl; | 
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|  | 96 | cout << _temperature << "-" << _numin << "-" << _numax << endl; | 
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|  | 97 | } | 
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|  | 98 |  | 
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| [669] | 99 | */ | 
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