1 | //--------------------------------------------------------------------------
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2 | // File and Version Information:
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3 | // $Id: derivblackbody.cc,v 1.6 2003-02-11 15:31:07 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 "machdefs.h"
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18 | #include <iostream>
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19 | #include <math.h>
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20 | #include "derivblackbody.h"
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21 |
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22 |
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23 |
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24 | /*! \class SOPHYA::DerivBlackBody
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25 | \ingroup SkyT
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26 | * This class corresponds to the emission spectrum of a
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27 | * dipole (since its emission spectrum is the derivation
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28 | * of a blackbody spectrum wrt the temperature).
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29 | */
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30 |
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31 | /*! Constructor: needs a temperature. Otherwise set to ConvTools::tcmb */
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32 | DerivBlackBody::DerivBlackBody(double temperature)
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33 | : RadSpectra(10., 10000.)
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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 | DerivBlackBody::~DerivBlackBody()
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40 | {
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41 | }
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42 |
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43 | /*!
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44 | The flux function is the derivation of the BlackBody
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45 | flux function wrt the temperature (used e.g. for a Dipole)
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46 | \f[
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47 | I_\nu = {2 h_{pl} (1.10^9*\nu)^3 {h_{pl}1.10^9*\nu \over k T^2}
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48 | {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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49 | \f]
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50 | */
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51 | double
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52 | DerivBlackBody::flux(double nu) const
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53 | {
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54 | if(nu < -1.e99) nu = -1.e99;
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55 | if(nu > 1.e99) nu = 1.e99;
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56 | double temperature = getTemperature();
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57 | if(nu==0.) return 0.;
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58 | double hpl = ConvTools::hpl;
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59 | double cel = ConvTools::cel;
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60 | double kb = ConvTools::kb;
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61 | double puiss1 = nu*pow(10.,9);
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62 | if(puiss1 > 1.e99) puiss1=1.e99;
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63 | if(puiss1 < -1.e99) puiss1=-1.e99;
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64 | double puiss2 = hpl*nu*pow(10.,9)/(kb*temperature);
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65 | if(puiss2 > 1.e99) puiss2=1.e99;
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66 | if(puiss2 < -1.e99) puiss2=-1.e99;
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67 |
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68 | double result=
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69 | (2*hpl* pow( puiss1 ,3))*(hpl*puiss1/kb)*(1/(temperature*temperature))
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70 | *exp(puiss2)
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71 | /(pow(cel,2)*pow(( (exp(puiss2)-1)),2));
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72 | // result = 1500e3*result/400e6;
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73 | return result;
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74 | }
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75 |
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76 |
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77 | void
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78 | DerivBlackBody::Print(ostream& os) const
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79 | {
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80 | os << "DerivBlackBody::Print Temp= " << getTemperature()
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81 | << " - Fmin,Fmax= " << minFreq() << "," << maxFreq() << endl;
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82 | os << "MeanFreq= " << meanFreq() << " Emission= " << flux(meanFreq()) << endl;
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83 | os << "PeakFreq= " << peakFreq() << " Emission= " << flux(peakFreq()) << endl;
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84 |
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85 | }
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86 |
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87 | /*
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88 | void
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89 | DerivBlackBody::WriteSelf(POutPersist& s)
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90 | {
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91 | s.PutR8(this->getTemperature());
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92 | s.PutR8(this->minFreq());
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93 | s.PutR8(this->maxFreq());
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94 | }
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95 |
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96 | void
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97 | DerivBlackBody::ReadSelf(PInPersist& s)
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98 | {
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99 | s.GetR8(_temperature);
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100 | s.GetR8(_numin);
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101 | s.GetR8(_numax);
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102 | cout << " Temperature - minFreq - maxFreq " << endl;
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103 | cout << _temperature << "-" << _numin << "-" << _numax << endl;
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104 | }
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105 |
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106 | */
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