| 1 | // Dominique YVON, CEA/DAPNIA/SPP 02/2000 | 
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| 2 |  | 
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| 3 | #ifndef LightDIFFDUST_SEEN | 
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| 4 | #define LightDIFFDUST_SEEN | 
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| 5 | #include "spheregorski.h" | 
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| 6 | #include "lightsrcsep.h" | 
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| 7 |  | 
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| 8 |  | 
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| 9 | class LightDiffDust:public LightSrcSep { | 
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| 10 | public: | 
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| 11 | LightDiffDust(int_4 nside); | 
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| 12 | virtual ~LightDiffDust(); | 
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| 13 | protected: | 
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| 14 | int nlat;           // Nlat de la carte gorsky de reference | 
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| 15 | double TDust;               // Temperature of dust | 
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| 16 | double fRef;                // Frequency Reference | 
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| 17 | double index;               // Index en frequence fitt sur le modle | 
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| 18 | double Hfraction; | 
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| 19 | double index2; | 
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| 20 | double CorrelatedfreeWeight; | 
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| 21 | double nuPlanckfRef; | 
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| 22 | SphereGorski<float>* pMap;         // Map units MJy from IRAS Data. | 
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| 23 |  | 
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| 24 | virtual double powerDensAmpli(double theta,double phi){ | 
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| 25 | return (*pMap)(theta,phi)*1.e-20*fRef; | 
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| 26 | // Return power density Amplidude at coordinates | 
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| 27 | // (W/m2/Hz/st) | 
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| 28 | } | 
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| 29 | virtual double spectre(double freq){ | 
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| 30 | /*  double temp=planckSpectrum(freq,TDust)/planckSpectrum(fRef,TDust) | 
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| 31 | *(1-Hfraction)* freq*freq/fRef/fRef; | 
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| 32 | return temp; | 
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| 33 | */ | 
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| 34 | double nuPnu= nuPlanck(freq)/nuPlanck(fRef) * (1.-Hfraction) * pow(freq/fRef,index) | 
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| 35 | + pow(freq/fRef,1+index2) * CorrelatedfreeWeight; | 
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| 36 | return nuPnu/freq; | 
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| 37 | } | 
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| 38 | inline double nuPlanck(double freq){ | 
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| 39 | return freq*planckSpectrum(freq,TDust); | 
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| 40 | } | 
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| 41 | }; | 
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| 42 |  | 
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| 43 | #endif | 
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| 44 |  | 
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