title test temperature of gas and dust in high energy density environment
c
c commands controlling continuum =========
table power law 
c intensity of incident radiation field set by its energy density
energy density temp 550 K
c
c commands for density & abundances =========
hden 5.0
init "ism.ini"
c Orion grains and abundances
abundances orion 
c
c commands controlling geometry  =========
stop zone 1
set drmax 10
c
c other commands for details     =========
c
c commands controlling output    =========
normalize to "O  8" 18.97A
save performance "grains_hot.per"
save monitors "grains_hot.asr" last 
save overview "grains_hot.ovr" last 
c
c commands giving the monitors    =========
// >>chng 07 dec 15, from 6.212 to 6.049, X-ray grain merge
monitor hydrogen 2 temperature 6.049
//
monitor grain potential  1  96.1 2
monitor grain potential  4  96.8 2
monitor grain potential  7  93.3 2
monitor grain potential 10  86.3 2
monitor grain potential 11 100.0 2
monitor grain potential 14 103.4 2
monitor grain potential 17 102.7 2
monitor grain potential 20  97.6 2
//
monitor grain temperature  1 1099 0.02
monitor grain temperature  4  998 0.02
monitor grain temperature  7  863 0.02
monitor grain temperature 10  712 0.02
monitor grain temperature 11 1366 0.02
monitor grain temperature 14 1201 0.02
monitor grain temperature 17 1039 0.02
monitor grain temperature 20  889 0.02
//
monitor line luminosity "GrGH" 0 -2.1261
monitor line luminosity "GrGC" 0 -2.1319
monitor line luminosity "GraI" 0  0.4222
monitor line luminosity "GraT" 0  0.4243
monitor line luminosity "GraC" 0 -1.8988
// >>chng 11 aug 05, from -3.318 to -4.538, make PRD redis func for h-like ions; LY_A func is now for H only
// >>chng 11 nov 16, from -4.538 to -4.513, adjust newmole monitors
monitor line luminosity "GraD" 0 -4.513
//
monitor line luminosity "FeKa" 1.78 -3.9067
c
c grains_hot.in
c class limit 
c ========================================
c 

This tests the grains in an extreme condition - irradiation by an AGN
near the illuminated face of the molecular torus.  The gas is 
predominantly heated by the grain electron photo-ejection.
