| 1 | //--------------------------------------------------------------------------
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| 2 | // File and Version Information:
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| 3 | //      $Id: derivblackbody.cc,v 1.7 2004-09-10 09:54:40 cmv Exp $
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| 4 | //
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| 5 | // Description:
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| 6 | //      Aim of the class: To give the derivative spectrum
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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 "sopnamsp.h"
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| 18 | #include "machdefs.h"
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| 19 | #include <iostream>
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| 20 | #include <math.h>
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| 21 | #include "derivblackbody.h"
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| 22 | 
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| 23 | 
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| 24 | 
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| 25 | /*! \class SOPHYA::DerivBlackBody 
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| 26 |   \ingroup SkyT
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| 27 |  * This class corresponds to the emission spectrum of a
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| 28 |  * dipole (since its emission spectrum is the derivation
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| 29 |  * of a blackbody spectrum wrt the temperature).
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| 30 |  */
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| 31 | 
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| 32 | /*! Constructor: needs a temperature. Otherwise set to ConvTools::tcmb */
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| 33 | DerivBlackBody::DerivBlackBody(double temperature)
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| 34 |   : RadSpectra(10., 10000.)
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| 35 | {
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| 36 |   _temperature = temperature;
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| 37 | }
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| 38 | 
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| 39 | 
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| 40 | DerivBlackBody::~DerivBlackBody()
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| 41 | {
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| 42 | }
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| 43 | 
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| 44 | /*!
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| 45 |   The flux function is the derivation of the BlackBody
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| 46 |   flux function wrt the temperature (used e.g. for a Dipole)
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| 47 |   \f[
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| 48 |   I_\nu = {2 h_{pl} (1.10^9*\nu)^3  {h_{pl}1.10^9*\nu \over k T^2}
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| 49 |         {e^{{h_{pl}(1.10^9*\nu) \over kT}}\over c^2 (e^{{h_{pl}(1.10^9*\nu) \over kT}} -1)^2}}
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| 50 |   \f]
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| 51 | */
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| 52 | double
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| 53 | DerivBlackBody::flux(double nu) const
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| 54 | {
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| 55 |   if(nu < -1.e99) nu = -1.e99;
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| 56 |   if(nu > 1.e99) nu = 1.e99;
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| 57 |   double temperature = getTemperature();
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| 58 |   if(nu==0.) return 0.;
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| 59 |   double hpl = ConvTools::hpl;
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| 60 |   double cel = ConvTools::cel;
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| 61 |   double kb  = ConvTools::kb;
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| 62 |   double puiss1 = nu*pow(10.,9);
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| 63 |   if(puiss1 >  1.e99)   puiss1=1.e99;
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| 64 |   if(puiss1 < -1.e99)   puiss1=-1.e99;
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| 65 |   double puiss2 = hpl*nu*pow(10.,9)/(kb*temperature);
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| 66 |   if(puiss2 >  1.e99)   puiss2=1.e99;
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| 67 |   if(puiss2 < -1.e99)   puiss2=-1.e99;
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| 68 |   
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| 69 |   double result=
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| 70 |    (2*hpl* pow( puiss1 ,3))*(hpl*puiss1/kb)*(1/(temperature*temperature))
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| 71 |     *exp(puiss2)
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| 72 |     /(pow(cel,2)*pow(( (exp(puiss2)-1)),2));
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| 73 |   //  result = 1500e3*result/400e6;
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| 74 |   return result;
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| 75 | }
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| 76 | 
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| 77 | 
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| 78 | void
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| 79 | DerivBlackBody::Print(ostream& os) const
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| 80 | {
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| 81 |   os << "DerivBlackBody::Print Temp= " << getTemperature() 
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| 82 |      << " - Fmin,Fmax= " << minFreq() << "," << maxFreq() << endl;
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| 83 |   os << "MeanFreq= " << meanFreq() << "  Emission= " << flux(meanFreq()) << endl;
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| 84 |   os << "PeakFreq= " << peakFreq() << "  Emission= " << flux(peakFreq()) << endl;
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| 85 | 
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| 86 | }
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| 87 | 
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| 88 | /*
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| 89 | void 
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| 90 | DerivBlackBody::WriteSelf(POutPersist& s)  
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| 91 | {
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| 92 |   s.PutR8(this->getTemperature());
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| 93 |   s.PutR8(this->minFreq());
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| 94 |   s.PutR8(this->maxFreq());
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| 95 | }
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| 96 | 
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| 97 | void
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| 98 | DerivBlackBody::ReadSelf(PInPersist& s)  
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| 99 | {
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| 100 |   s.GetR8(_temperature);
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| 101 |   s.GetR8(_numin);
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| 102 |   s.GetR8(_numax);
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| 103 |   cout << " Temperature - minFreq - maxFreq " << endl; 
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| 104 |   cout << _temperature << "-" << _numin << "-" << _numax << endl;
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| 105 | }
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| 106 | 
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| 107 | */
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