source: Sophya/trunk/SophyaLib/SkyT/derivblackbody.cc@ 3809

Last change on this file since 3809 was 2615, checked in by cmv, 21 years ago

using namespace sophya enleve de machdefs.h, nouveau sopnamsp.h cmv 10/09/2004

File size: 2.8 KB
RevLine 
[879]1//--------------------------------------------------------------------------
2// File and Version Information:
[2615]3// $Id: derivblackbody.cc,v 1.7 2004-09-10 09:54:40 cmv Exp $
[879]4//
5// Description:
6// Aim of the class: To give the derivative spectrum
7// The unity used here is W/m^2/Hz/sr
8//
9// History (add to end):
10// Sophie Oct, 1999 - creation
11//
12//------------------------------------------------------------------------
13
14//---------------
15// C++ Headers --
16//---------------
[2615]17#include "sopnamsp.h"
[879]18#include "machdefs.h"
[2322]19#include <iostream>
[879]20#include <math.h>
21#include "derivblackbody.h"
22
[909]23
24
[927]25/*! \class SOPHYA::DerivBlackBody
26 \ingroup SkyT
[909]27 * This class corresponds to the emission spectrum of a
28 * dipole (since its emission spectrum is the derivation
29 * of a blackbody spectrum wrt the temperature).
30 */
31
32/*! Constructor: needs a temperature. Otherwise set to ConvTools::tcmb */
[879]33DerivBlackBody::DerivBlackBody(double temperature)
34 : RadSpectra(10., 10000.)
35{
36 _temperature = temperature;
37}
38
39
40DerivBlackBody::~DerivBlackBody()
41{
42}
43
[909]44/*!
45 The flux function is the derivation of the BlackBody
46 flux function wrt the temperature (used e.g. for a Dipole)
47 \f[
48 I_\nu = {2 h_{pl} (1.10^9*\nu)^3 {h_{pl}1.10^9*\nu \over k T^2}
49 {e^{{h_{pl}(1.10^9*\nu) \over kT}}\over c^2 (e^{{h_{pl}(1.10^9*\nu) \over kT}} -1)^2}}
50 \f]
51*/
[879]52double
53DerivBlackBody::flux(double nu) const
54{
55 if(nu < -1.e99) nu = -1.e99;
56 if(nu > 1.e99) nu = 1.e99;
57 double temperature = getTemperature();
58 if(nu==0.) return 0.;
59 double hpl = ConvTools::hpl;
60 double cel = ConvTools::cel;
61 double kb = ConvTools::kb;
[2144]62 double puiss1 = nu*pow(10.,9);
[879]63 if(puiss1 > 1.e99) puiss1=1.e99;
64 if(puiss1 < -1.e99) puiss1=-1.e99;
[2144]65 double puiss2 = hpl*nu*pow(10.,9)/(kb*temperature);
[879]66 if(puiss2 > 1.e99) puiss2=1.e99;
67 if(puiss2 < -1.e99) puiss2=-1.e99;
68
69 double result=
70 (2*hpl* pow( puiss1 ,3))*(hpl*puiss1/kb)*(1/(temperature*temperature))
71 *exp(puiss2)
72 /(pow(cel,2)*pow(( (exp(puiss2)-1)),2));
[893]73 // result = 1500e3*result/400e6;
[879]74 return result;
75}
76
77
78void
79DerivBlackBody::Print(ostream& os) const
80{
81 os << "DerivBlackBody::Print Temp= " << getTemperature()
82 << " - Fmin,Fmax= " << minFreq() << "," << maxFreq() << endl;
83 os << "MeanFreq= " << meanFreq() << " Emission= " << flux(meanFreq()) << endl;
84 os << "PeakFreq= " << peakFreq() << " Emission= " << flux(peakFreq()) << endl;
85
86}
87
88/*
89void
90DerivBlackBody::WriteSelf(POutPersist& s)
91{
92 s.PutR8(this->getTemperature());
93 s.PutR8(this->minFreq());
94 s.PutR8(this->maxFreq());
95}
96
97void
98DerivBlackBody::ReadSelf(PInPersist& s)
99{
100 s.GetR8(_temperature);
101 s.GetR8(_numin);
102 s.GetR8(_numax);
103 cout << " Temperature - minFreq - maxFreq " << endl;
104 cout << _temperature << "-" << _numin << "-" << _numax << endl;
105}
106
107*/
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