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    Cloudy
    
   Spectral Synthesis Code for Astrophysics 
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Public Member Functions | |
| void | clear () | 
Public Attributes | |
| double | a [NSD] | 
| double | lim [2] | 
| double | clim [2] | 
| vector< double > | xx | 
| vector< double > | aa | 
| vector< double > | rr | 
| vector< double > | ww | 
| double | unity | 
| double | unity_bin | 
| double | cSize | 
| double | radius | 
| double | area | 
| double | vol | 
| vector< double > | ln_a | 
| vector< double > | ln_a4dNda | 
| sd_type | sdCase | 
| long int | nCarbon | 
| long int | magic | 
| long int | cPart | 
| long int | nPart | 
| long int | nmul | 
| long int | nn | 
| long int | npts | 
| bool | lgLogScale | 
Private Member Functions | |
| void | p_clear1 () | 
      
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  inline | 
      
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  inlineprivate | 
| double sd_data::a[NSD] | 
parameters for size distribution
Referenced by mie_auxiliary(), mie_cs_size_distr(), mie_read_szd(), and size_distr().
| vector<double> sd_data::aa | 
aa[nn]: weights for Gauss quadrature on [-1,1]
Referenced by mie_integrate(), and p_clear1().
| double sd_data::area | 
average grain surface area for current bin <4pi*a^2>
Referenced by mie_auxiliary(), mie_integrate(), and mie_write_opc().
| double sd_data::clim[2] | 
holds lower and upper size limit for current bin
Referenced by mie_auxiliary(), mie_integrate(), mie_step(), and mie_write_opc().
| long int sd_data::cPart | 
current partition no. for size distribution
Referenced by mie_auxiliary(), and mie_write_opc().
| double sd_data::cSize | 
the grain size currently being used for the calculations
Referenced by mie_cs(), mie_cs_size_distr(), mie_step(), pah1_fun(), pah2_fun(), and pah3_fun().
| bool sd_data::lgLogScale | 
use logarithmic mesh for integration over size ?
Referenced by mie_auxiliary(), mie_integrate(), and mie_write_opc().
| double sd_data::lim[2] | 
holds lower and upper size limit for entire distribution
Referenced by mie_auxiliary(), mie_read_szd(), mie_write_opc(), search_limit(), and size_distr().
| vector<double> sd_data::ln_a | 
ln(a)[npts]: log of grain radii for user-supplied size distr
Referenced by mie_read_szd(), p_clear1(), and size_distr().
| vector<double> sd_data::ln_a4dNda | 
ln(a^4*dN/da)[npts]: log of user-supplied size distr
Referenced by mie_read_szd(), p_clear1(), and size_distr().
| long int sd_data::magic | 
magic number
Referenced by mie_read_szd(), and mie_write_opc().
| long int sd_data::nCarbon | 
number of carbon atoms requested in SD_NR_CARBON file
Referenced by mie_auxiliary(), and mie_read_szd().
| long int sd_data::nmul | 
multiplier for obtaining no. of abscissas in gaussian quadrature
Referenced by mie_auxiliary(), and mie_integrate().
| long int sd_data::nn | 
no. of abscissas used in gaussian quadrature (per partition)
Referenced by mie_integrate().
| long int sd_data::nPart | 
total no. of partitions for size distribution
Referenced by mie_auxiliary(), and mie_write_opc().
| long int sd_data::npts | 
no. of points in user-supplied size distr
Referenced by mie_read_szd(), and size_distr().
| double sd_data::radius | 
average grain radius for current bin
Referenced by mie_auxiliary(), mie_integrate(), and mie_write_opc().
| vector<double> sd_data::rr | 
rr[nn]: abcissas for Gauss quadrature
Referenced by mie_integrate(), and p_clear1().
| sd_type sd_data::sdCase | 
SD_SINGLE_SIZE, SD_POWERLAW, ...
Referenced by mie_auxiliary(), mie_cs_size_distr(), mie_read_szd(), mie_write_opc(), and size_distr().
| double sd_data::unity | 
normalization for integrals over size distribution
Referenced by mie_auxiliary(), and mie_write_opc().
| double sd_data::unity_bin | 
normalization for integrals over size distribution
Referenced by mie_auxiliary(), and mie_write_opc().
| double sd_data::vol | 
average grain volume for current bin <4pi/3*a^3>
Referenced by mie_auxiliary(), mie_integrate(), and mie_write_opc().
| vector<double> sd_data::ww | 
ww[nn]: weights for Gauss quadrature
Referenced by mie_integrate(), and p_clear1().
| vector<double> sd_data::xx | 
xx[nn]: abcissas for Gauss quadrature on [-1,1]
Referenced by mie_integrate(), and p_clear1().