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dense_parametric_wind.cpp
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/* This file is part of Cloudy and is copyright (C)1978-2013 by Gary J. Ferland and
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* others. For conditions of distribution and use see copyright notice in license.txt */
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#include "
cddefines.h
"
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#include "
dense.h
"
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#include "
radius.h
"
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/*dense_parametric_wind called by dlaw command, returns density for any density law */
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double
dense_parametric_wind
(
double
rad)
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{
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/* >> refer wind profile Springmann, U., 1994, A&A, 289, 505 */
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// SOLAR_MASS / 3e7 converts from M_solar/year to g/s
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double
Mdot =
dense
.
DensityLaw
[0] *
SOLAR_MASS
/ 3e7;
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double
v_inf =
dense
.
DensityLaw
[1] * 1e5;
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double
Beta2 =
dense
.
DensityLaw
[2];
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double
Beta1 =
dense
.
DensityLaw
[3];
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double
v_0 =
dense
.
DensityLaw
[4] * 1e5;
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double
v_star =
dense
.
DensityLaw
[5] * 1e5;
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double
r_star =
radius
.
rinner
;
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double
x =
MIN2
( 0.01, 1. - r_star/rad );
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double
v_r = v_star + (v_inf - v_0) * sqrt( Beta1 * x + (1.-Beta1) * pow(x, Beta2) );
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double
mu = 1.;
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if
(
dense
.
wmole
> 0. )
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mu =
dense
.
wmole
;
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double
density = Mdot / (
PI4
*
ATOMIC_MASS_UNIT
* mu * pow(rad, 2.) * v_r);
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return
density;
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}
cddefines.h
MIN2
#define MIN2
Definition:
cddefines.h:761
dense
t_dense dense
Definition:
dense.cpp:24
dense.h
dense_parametric_wind
double dense_parametric_wind(double rad)
Definition:
dense_parametric_wind.cpp:8
SOLAR_MASS
UNUSED const double SOLAR_MASS
Definition:
physconst.h:71
PI4
UNUSED const double PI4
Definition:
physconst.h:35
ATOMIC_MASS_UNIT
UNUSED const double ATOMIC_MASS_UNIT
Definition:
physconst.h:88
radius
t_radius radius
Definition:
radius.cpp:5
radius.h
t_dense::DensityLaw
double DensityLaw[10]
Definition:
dense.h:173
t_dense::wmole
realnum wmole
Definition:
dense.h:101
t_radius::rinner
double rinner
Definition:
radius.h:22
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