Cloudy & Associates
Skip to content
GitLab
Menu
Projects
Groups
Snippets
Help
Help
Support
Community forum
Keyboard shortcuts
?
Submit feedback
Sign in
Toggle navigation
Menu
Open sidebar
cloudy
cloudy
Commits
b0375930
Commit
b0375930
authored
Oct 29, 2021
by
Marios Chatzikos
Browse files
Merge branch 'master' into pseudo
parents
e5632944
391f6504
Changes
9
Hide whitespace changes
Inline
Side-by-side
tsuite/auto
/star_kurucz_35000.dat
→
data
/star_kurucz_35000.dat
View file @
b0375930
File moved
tsuite/auto
/star_kurucz_39600.dat
→
data
/star_kurucz_39600.dat
View file @
b0375930
File moved
tsuite/auto
/star_mihalas_46000.dat
→
data
/star_mihalas_46000.dat
View file @
b0375930
File moved
docs/latex/QuickStart/VeuszCookbook.tex
View file @
b0375930
...
...
@@ -229,6 +229,7 @@ You can also place graphs within a grid widget to get an arrangement of separate
Figure
\ref
{
fig:orion
_
hii
_
pdr
_
pp
}
shows an example,
taken from the Orion HII region / PDR simulation, of a nested plot.
\begin{figure}
\begin{center}
\includegraphics
[clip=on,width=0.8\columnwidth,height=0.8\textheight,keepaspectratio]
{
orion
_
hii
_
pdr
_
pp
}
...
...
@@ -239,4 +240,13 @@ Orion H II region / PDR.}
\label
{
fig:orion
_
hii
_
pdr
_
pp
}
\end{figure}
\subsection
{
Documenting your work
}
The Properties widget includes a Notes field that can be used to keep a history of the
data behind a plot.
This is useful so that you can come back to a project after some time and recover
the history of the work leading up to a result or the location of the helper files that were used
along the way.
%\end{document}
docs/latex/frontis_common.tex
View file @
b0375930
{
\small
\noindent
{
\em
Software:
}
Copyright
\copyright\
1978-20
19
Gary J. Ferland and others. All rights reserved.
{
\em
Software:
}
Copyright
\copyright\
1978-20
22
Gary J. Ferland and others. All rights reserved.
\vspace
{
1em
}
...
...
@@ -44,7 +44,7 @@ to the following FreeBSD format documentation license:
\vspace
{
1em
}
\noindent
{
\em
Documentation:
}
Copyright
\copyright\
1978--20
19
Gary J. Ferland and others. All rights reserved.
{
\em
Documentation:
}
Copyright
\copyright\
1978--20
22
Gary J. Ferland and others. All rights reserved.
\vspace
{
1em
}
...
...
source/cool_eval.cpp
View file @
b0375930
...
...
@@ -1293,9 +1293,9 @@ STATIC double CoolH2_GA08 ( double Temp )
{
DEBUG_ENTRY
(
"CoolH2_GA08()"
);
double
x_para
=
h2
.
para_density
/
dense
.
gas_phase
[
ipHYDROGEN
];
double
x_ortho
=
h2
.
ortho_density
/
dense
.
gas_phase
[
ipHYDROGEN
];
double
f_para
=
h2
.
para_density
/
(
h2
.
para_density
+
h2
.
ortho_density
);
double
x_para
=
safe_div
(
h2
.
para_density
,
double
(
dense
.
gas_phase
[
ipHYDROGEN
]
)
)
;
double
x_ortho
=
safe_div
(
h2
.
ortho_density
,
double
(
dense
.
gas_phase
[
ipHYDROGEN
]
)
)
;
double
f_para
=
safe_div
(
h2
.
para_density
,
h2
.
para_density
+
h2
.
ortho_density
);
double
f_ortho
=
1.
-
f_para
;
/* Collisions with atomic H */
...
...
@@ -1354,14 +1354,10 @@ STATIC double CoolH2_GA08 ( double Temp )
}
}
/* NB NB NB
*
* The interpolation below will fail if the high density cooling is 0,
* that is, the total cooling will be 0, even if the low-density cooling
* is not. This may happen if permitted by the function that computes
* LTE cooling, and/or the tabulated data (see definition of
* interpolate_LTE_Cooling() and associated data file). */
return
cooling_high
/
(
1.
+
cooling_high
/
cooling_low
);
// originally cooling_high / (1. + cooling_high / cooling_low)
// See Eq. (39) therein
//
return
safe_div
(
cooling_low
*
cooling_high
,
cooling_low
+
cooling_high
);
}
STATIC
void
CoolHyperfine
(
void
)
...
...
source/hextra.h
View file @
b0375930
...
...
@@ -109,7 +109,7 @@ struct t_hextra : public module {
hextra.background_density = 1.99e-9f;*/
/* >>chng 05 apr 16, to get proper ionization rate in ism_set_cr_rate, where
* H is forced to be fully atomic, no molecules, density from 1.99 to 2.15 */
/* >>chng
0
2 apr 05, update to
/* >>chng
1
2 apr 05, update to
* >>refer cosmic ray ionization Indriolo, N., Geballe, T., Oka, T., & McCall, B.J. 2007, ApJ, 671, 1736
*/
background_density
=
2.15e-9
f
*
7
.
9
f
;
...
...
tsuite/slow/h2_th85orion.in
View file @
b0375930
...
...
@@ -39,7 +39,7 @@ normalize to "C 2" 157.636m
sphere
## >>chng 16 apr 14, had been case B, this gets same effect with
## no large Lyman optical depths
D
atabase H-like Lyman pumping off
d
atabase H-like Lyman pumping off
cosmic rays, background
##
## stopping criteria
...
...
tsuite/slow/star_kurucz_39600.dat
deleted
120000 → 0
View file @
e5632944
../auto/star_kurucz_39600.dat
\ No newline at end of file
Write
Preview
Markdown
is supported
0%
Try again
or
attach a new file
.
Attach a file
Cancel
You are about to add
0
people
to the discussion. Proceed with caution.
Finish editing this message first!
Cancel
Please
register
or
sign in
to comment