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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().