1 | #include "sopnamsp.h"
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2 | #include "alm.h"
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3 |
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4 |
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5 | /*!
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6 | \class Alm
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7 | \ingroup Samba
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8 | Class for manipulating the coefficients \f$a_{lm}\f$ of the development
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9 | in spherical harmonics of a function efined on a sphere.
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10 | */
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11 |
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12 | /*!
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13 | fwhm specifies the gaussian beam half witdh in arc.minutes
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14 | */
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15 | template <class T>
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16 | Alm<T>::Alm(const TVector<T>& clin, const r_8 fwhm)
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17 |
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18 | {
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19 | int_4 nlmax= clin.NElts()-1;
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20 |
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21 | //alm.ReSize(nlmax);
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22 | this->ReSizeRow(nlmax+1);
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23 | RandomGenerator rg(1, false);
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24 | GenFromCl(clin, fwhm, rg);
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25 | }
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26 |
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27 | /*!
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28 | fwhm specifies the gaussian beam half witdh in arc.minutes
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29 | */
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30 | template <class T>
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31 | Alm<T>::Alm(const TVector<T>& clin, const r_8 fwhm, RandomGenerator & rg)
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32 | {
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33 | int_4 nlmax= clin.NElts()-1;
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34 |
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35 | //alm.ReSize(nlmax);
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36 | this->ReSizeRow(nlmax+1);
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37 | GenFromCl(clin, fwhm, rg);
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38 | }
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39 |
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40 |
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41 |
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42 | template <class T>
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43 | void Alm<T>::GenFromCl(const TVector<T> & clin, const r_8 fwhm, RandomGenerator & rg)
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44 | {
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45 | /*=======================================================================
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46 | creates the a_lm from the power spectrum,
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47 | assuming they are gaussian and complex
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48 | with a variance given by C(l)
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49 |
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50 | the input file should contain : l and C(l) with *consecutive* l's
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51 | (missing C(l) are put to 0.)
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52 |
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53 | because the map is real we have : a_l-m = (-)^m conjug(a_lm)
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54 | so we actually compute them only for m >= 0
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55 |
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56 | =======================================================================*/
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57 | int_4 nlmax= clin.NElts()-1;
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58 |
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59 | r_8 sig_smooth = fwhm/sqrt(8.*log(2.))/(60.*180.)* M_PI;
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60 | int_4 n_l = nlmax+1;
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61 |
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62 |
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63 | // --- smoothes the initial power spectrum ---
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64 | TVector<T> cl(clin, false);
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65 | int l;
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66 | for (l=0;l<n_l;l++)
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67 | {
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68 | r_8 gauss=exp(-l*(l+1.)*sig_smooth*sig_smooth);
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69 | cl(l)*=(T)gauss;
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70 | }
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71 |
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72 |
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73 | // --- generates randomly the alm according to their power spectrum ---
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74 | r_8 hsqrt2 = 1.0 / Rac2;
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75 |
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76 | for (l=0;l<n_l;l++)
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77 | {
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78 | T rms=sqrt(cl(l));
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79 | // ------ m = 0 ------
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80 | complex<T> zeta1((T)rg.Gaussian() );
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81 | (*this)(l,0) = zeta1 * rms;
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82 |
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83 | //------ m > 0 ------
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84 | for (int m=1;m<=l;m++)
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85 | {
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86 | complex<T> aux1(hsqrt2);
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87 | complex<T> aux2((T)rg.Gaussian() , (T)rg.Gaussian() );
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88 | zeta1=aux1*aux2;
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89 | (*this)(l,m)=rms*zeta1;
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90 | }
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91 | }
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92 | }
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93 |
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94 |
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95 | template <class T>
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96 | TVector<T> Alm<T>::powerSpectrum() const
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97 | {
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98 | int_4 nlmax=Lmax();
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99 |
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100 | TVector<T> powsp(nlmax+1);
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101 |
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102 | for (int l=0; l<=nlmax;l++)
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103 | {
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104 | powsp(l)=( (*this)(l,0) ).real()*( (*this)(l,0) ).real();
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105 | for (int m=1; m<=l; m++)
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106 | {
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107 | powsp(l)+=2.*( (*this)(l,m).real()*(*this)(l,m).real()+
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108 | (*this)(l,m).imag()*(*this)(l,m).imag() );
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109 | }
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110 | powsp(l)/=(2.*l+1.);
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111 | }
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112 | return powsp;
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113 | }
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114 |
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115 | /*!
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116 | \class Bm
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117 | \ingroup Samba
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118 | Class for a vector with an index running from \f$-m_{max}\f$ to \f$+m_{max}\f$
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119 | (then the size of the vector will be actually \f$2m_{max}+1)\f$.
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120 | This class is used by the spherical harmonics transform server
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121 | */
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122 |
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123 |
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124 | #ifdef __CXX_PRAGMA_TEMPLATES__
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125 | #pragma define_template Alm<r_8>
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126 | #pragma define_template Alm<r_4>
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127 | #endif
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128 | #if defined(ANSI_TEMPLATES) || defined(GNU_TEMPLATES)
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129 | template class SOPHYA::Alm<r_8>;
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130 | template class SOPHYA::Alm<r_4>;
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131 | #endif
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