Commit f03174cd authored by Michal Dovčiak's avatar Michal Dovčiak
Browse files

Small update in documentation.

parent 89e58eb6
......@@ -171,16 +171,17 @@ Definition in XSPEC
source is located (GM/c^(2))
* **par10 ... PhoIndex**
- power-law energy index of the primary flux
* **par11 ... Np**
- dN/dt/dΩ, the intrinsic local (if negative) or the observed
* **par11 ... L/L~Edd~**
- dE/dt;, the intrinsic local (if negative) or the observed
(if positive) primary isotropic flux in the X-ray energy range 2-10keV
in units of L~Edd~
* **par12 ... NpNr**
- ratio of the primary to the reflected normalization
- 1: self-consistent model for isotropic primary source
- 0: only reflection, primary source is hidden
- if positive then Np (par11) means the luminosity towards the observer
- if negative then Np (par11) means the luminosity towards the disc
- if positive then L/L~Edd~ (par11) means the luminosity towards the
observer
- if negative then L/L~Edd~ (par11) means the luminosity towards the disc
* **par13 ... nH0**
- density profile normalization in 10^15 cm^(-3)
* **par14 ... q_n**
......
......@@ -53,16 +53,16 @@
* par9 ... height - height on the axis (measured from the center) at which
* the primary source is located (GM/c^2)
* par10 ... PhoIndex - power-law energy index of the primary flux
* par11 ... Np - dN/dt/dOmega, the intrinsic local (if negative) or the
* par11 ... L/Ledd - dE/dt, the intrinsic local (if negative) or the
* observed (if positive) primary isotropic flux in the
* X-ray energy range 2-10keV in units of Ledd
* par12 ... NpNr - ratio of the primary to the reflected normalization
* 1 - self-consistent model for isotropic primary source
* 0 - only reflection, primary source is hidden
* - if negative then Np (par11) means the luminosity towards
* the disc
* - if positive then Np (par11) means the luminosity towards
* the observer
* - if negative then L/Ledd (par11) means the luminosity
* towards the disc
* - if positive then L/Ledd (par11) means the luminosity
* towards the observer
* par13 ... nH0 - density profile normalization in 10^15 cm^(-3)
* par14 ... q_n - radial power-law density profile
* par15 ... abun - Fe abundance (in solar abundance)
......@@ -77,10 +77,12 @@
* rcloud, i.e. only the radiation behind the cloud is
* computed
* par19 ... zshift - overall Doppler shift
* par20 ... limb - defines fits file with tables
* 0 -> for isotropic emission (flux ~ 1)
* 1 -> for Laor's limb darkening (flux ~ (1+2.06*mu))
* 2 -> for Haardt's limb brightening (flux ~ ln (1+1/mu))
* par20 ... limb - limb darkening/brightening law (emission directionality)
* - if = 0 the local emisivity is not multiplied by anything
* - if = 1 the local emisivity is multiplied by 1+2.06*mu
* (limb darkening)
* - if = 2 the local emisivity is multiplied by ln(1+1/mu)
* (limb brightening)
* par21 ... tab - which reflion table to use
* 1 -> reflion (the old one, lower cut-off energy at 1eV,
* not good for PhoIndex > 2)
......@@ -92,9 +94,8 @@
* 2 -> use the Xi correspondent to the computed normalization
* of the incident flux, i.e. do not shift the cut-offs
* when computing the total incident intensity
* par23 ... ntable - defines fits file with tables (0 <= ntable <= 99)
* by default only the tables with ntable=80 are
* correct for this model
* par23 ... ntable - table of relativistic transfer functions used in the model
* (defines fits file with tables), 0<= ntable <= 99
* par24 ... nradius - number of grid points in radius
* - if negative than the number of radial grid points is
* dependent on height as -nradius / height^0.66
......@@ -381,7 +382,7 @@ param[ 6] = 360.; // dphi
param[ 7] = 0.1; // M/M8
param[ 8] = 3.; // height
param[ 9] = 2.; // PhoIndex
param[10] = 0.001; // Np
param[10] = 0.001; // L/Ledd
param[11] = 1.; // NpNr
param[12] = 1.; // nH0
param[13] = 0.; // q_n
......@@ -675,8 +676,8 @@ else {
}
// PhoIndex - power-law energy index of the lamp emission
gamma0 = param[9];
// Np - dN/dt/dOmega primary isotropic flux in Eddington luminosity
// as seen by the disc
// L/Ledd - dE/dt primary isotropic flux in Eddington luminosity as seen by the
// disc
Np = param[10];
// Np:Nr - ratio of the primary to the reflected normalization
NpNr = param[11];
......
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