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Commit 796c27f8 authored by Andrew Strong's avatar Andrew Strong
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GALDEF

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Title = copy of 55_z04LMo7S but with pion production matrices:pi0_decay=2 QGSJET : 10,11,12 reduced Ekin max, increased E_gamma_min to avoid nan
Title = which was copy of 54_z04LMS with same healpix order 7
Title = which was copy of 54_z02G4c5MS but with Lorimer pulsars (but flat R=10-15 kpc) instead of Gaussian source distribution
Title = which was copy of 54_z10G4c5mS but with B_field =070500030 and wideband gammas and finer sync.all compatible with z02,z04*MS Ekin_min=100 MeV 10 per decade CR and gamma
Title = which was copy of 54_z10G4c5kS but no flattening of Gaussian source in outer Galaxy
Title = which was copy of 54_z10G4c5rS but galprop r381 new CO analytical model, EBV: 2mag cut, no b cut
Title = which was copy of 54_z10FenprS but with Gaussian source, 4.5 kpc flat beyond 8.5 kpc
Title = which was copy of 54_z04FenprS but zh=10 and appropriate Dxx
Title = which was copy of 54_z04FenpDS but with new CO, type 3 ISRF. Reference models for paper 2.
Title = which was copy of 54_z04FelD7S but with Fermi electrons unscaled, protons unscaled, Gaensler HII. B_field and gas model parameters added
Title = which was copy of 54_z04Feld7S but with E(B-V) local HI ring with pos and neg residuals, bmin=5, E(B-V) max =5
Title = which was copy of 54_z04Felh7S but with E(B-V) local HI ring as in z04epmdGS
Title = which was copy of 54_87Xexph7S but with Fermi electrons unscaled, protons*1.15. galprop r275
Title = which was copy of 54_86Xexph7S but with energy range 50 MeV - 100 GeV, 30 bins as requested by Seth. integration mode changed to 0 to avoid bremss wiggles
Title = which was copy of 54_85Xexph7S but with protons factor 1.35 instead of 1.30
Title = which was copy of 54_82Xexph7S but with protons factor 1.30 instead of 1.15
Title = which was copy of 54_81Xexph7S but with moment-masked CO dataset
Title = which was copy of 54_77Xexph7S but with CR gradient adjusted to give more in outer Galaxy see Fermi paper 2 gradplot.pro
Title = which was copy of 54_77Xvarh7S but with exponential Xco based on recent Fermi results: 10^(-0.4+0.066*R)
Title = which was copy of 54_72Xvarh7S but with new CO map from Gulli rbands_co9 and galprop r223 with reinstated store_IC_skymap
Title = which was copy of 54_71Xvarh7S but with p,He and electrons scaled based on gardian all-sky fit, p,He factor=1.15, electrons factor=1.75
Title = which was copy of 54_70Xvarh7S but with electron injection spectrum 2.42
Title = which was copy of 54_5FXvarh7S but with electron injection adjusted to Fermi
Title = which was copy of 54_5EXvarh7S but with Kamae pion-decay instead of old formalism
Title = which was copy of 54_5BXvarh7S but with electrons factor 0.4e-9 instead of 0.6e-9 (i.e. original conventional model)
Title = which was copy of 54_5Avarh7S but with higher gamma-ray energy resolution
Title = which was copy of 54_56varh7S but with new gradient and electrons *1.5 from gardian 4-ring fit using dubois to 22 Aug
Title = which was copy of 54_55Xvarh7S but with Ekin_max=1.0e9
Title = which was copy of 54_610202h7S but n_X_CO=9 for standard variation of X_CO and source under v54, propagation parameters from galdef_53_5102229RG
Title = with e+e- secondaries and smaller E_gamma_factor than 54_54Xvarh7S
n_spatial_dimensions = 2
r_min =00.0 min r
r_max =20.00 max r
dr = 1.0 delta r
z_min =-04.0 min z
z_max =+04.0 max z
dz = 0.1 delta z
x_min =-10.0 min x
x_max =+10.0 max x
dx = 1.0 delta x
y_min =-10.0 min y
y_max =+10.0 max y
dy = 1.0 delta y
p_min =1000 min momentum (MV)
p_max =4000 max momentum
p_factor =1.50 momentum factor
Ekin_min =1.0e2 min kinetic energy per nucleon (MeV)
Ekin_max =1.0e8 1.0e9 max kinetic energy per nucleon 1e9 gives nan or inf for pi0 method 10
Ekin_factor =1.2589254 1.2 kinetic energy per nucleon factor
p_Ekin_grid = Ekin p||Ekin alignment
E_gamma_min = 1.0e-2 1.0 1.0e-2 min gamma-ray energy (MeV) 1e-2 gives nan for pi0 method 10
E_gamma_max = 1.0e+7 max gamma-ray energy (MeV)
E_gamma_factor = 1.2589254 1.2996566 gamma-ray energy factor
integration_mode = 0 integr.over part.spec.: =1-old E*logE; =0-PL analyt.
nu_synch_min = 1.0e6 min synchrotron frequency (Hz)
nu_synch_max = 1.0e12 max synchrotron frequency (Hz)
nu_synch_factor = 1.1 synchrotron frequency factor
long_min = 0.25 gamma-ray intensity skymap longitude minimum (deg); 0 -automatic binning required to get correct results!
long_max =359.75 gamma-ray intensity skymap longitude maximum (deg); 360 -automatic binning
lat_min =-89.75 gamma-ray intensity skymap latitude minimum (deg); -90 -automatic binning
lat_max =+89.75 gamma-ray intensity skymap latitude maximum (deg); +90 -automatic binning
d_long = 0.5 gamma-ray intensity skymap longitude binsize (deg)
d_lat = 0.5 gamma-ray intensity skymap latitude binsize (deg)
healpix_order = 7 order for healpix skymaps. 7 gives ~0.5 deg and it changes by an order of 2
lat_substep_number = 1 latitude bin splitting (0,1=no split, 2=split in 2...)
LoS_step = 0.01 kpc, Line of Sight (LoS) integration step
LoS_substep_number = 1 number of substeps per LoS integration step (0,1=no substeps)
D0_xx = 5.8e28 diffusion coefficient at reference rigidity
D_rigid_br =4.0e3 reference rigidity for diffusion coefficient in MV
D_g_1 = 0.33 diffusion coefficient index below reference rigidity
D_g_2 = 0.33 diffusion coefficient index above reference rigidity
diff_reacc =1 0=no reacc.; 1,2=incl.diff.reacc.; -1==beta^3 Dxx; 11=Kolmogorov+damping; 12=Kraichnan+damping
v_Alfven =30. Alfven speed in km s-1
damping_p0 = 1.e6 MV -some rigidity (where CR density is low)
damping_const_G = 0.02 a const derived from fitting B/C
damping_max_path_L = 3.e21 Lmax~1 kpc, max free path
convection =0 1=include convection
v0_conv =0. km s-1 v_conv=v0_conv+dvdz_conv*dz
dvdz_conv =10. km s-1 kpc-1 v_conv=v0_conv+dvdz_conv*dz
nuc_rigid_br = 9.0e3 reference rigidity for nucleus injection index in MV
nuc_g_1 =1.98 nucleus injection index below reference rigidity
nuc_g_2 =2.42 nucleus injection index index above reference rigidity
inj_spectrum_type = rigidity rigidity||beta_rig||Etot nucleon injection spectrum type
electron_g_0 =1.60 electron injection index below electron_rigid_br0
electron_rigid_br0 =4.0e3 reference rigidity0 for electron injection index in MV
electron_g_1 =2.42 2.3 2.54 electron injection index below reference rigidity
electron_rigid_br =1.0e9 reference rigidity for electron injection index in MV
electron_g_2 =5.0 electron injection index index above reference rigidity
He_H_ratio = 0.11 He/H of ISM, by number
n_X_CO = 10 an option to select functional dependence of X_CO=X_CO(R) 0=constant as below, 9=standard variation as in A&A 2004 paper 10=an exponential
X_CO = 1.9E20 conversion factor from CO integrated temperature to H2 column density
nHI_model = 1 selection of HI gas density model (not yet implemented)
nH2_model = 1 selection of H2 gas density model (not yet implemented)
nHII_model = 3 selection of HII gas density model 1=Cordes et al 1991 2=NE2001 3 = Gaensler etal 2008
COR_filename = rbands_co10mm_v2_2001_qdeg.fits.gz rbands_co10mm_2001_qdeg.fits.gz rbands_co9_qdeg.fits.gz
HIR_filename = rbands_hi12_v2_qdeg_zmax1_Ts125_EBV2.0_localring_4.fits rbands_hi12_v2_qdeg_zmax1_Ts125_EBV_localring_3.fits rbands_hi12_qdeg_zmax1.fits.gz
B_field_model = 070500030 bbbrrrzzz bbb=10*B(0) rrr=10*rscale zzz=10*zscale
B_field_name = galprop_original han_ran 3D models:han .... galprop_original: exponential model as in original (parameters Bo, rscale, zscale)
n_B_field_parameters = 10 number of B-field parameters (must be 10 at present)
B_field_parameters = 9.0e-6,65.0,-8.5,12.26,5.00e-6,0.0,0.0,0.0,0.0,0.2 parameters for 3D models, meaning depends on the model
ISRF_file = ISRF/Standard/Standard.dat ISRF_RMax20_ZMax5_DR0.5_DZ0.1_MW_BB_24092007.fits input ISRF file
ISRF_filetype = 3 2 3=new 2=old NB this changed from 1 to 2 for the same file type
ISRF_healpixOrder = 3 for output of ISRF skymaps
ISRF_factors = 1.0,1.0,1.0 ISRF factors for IC calculation: optical, FIR, CMB
fragmentation =1 1=include fragmentation
momentum_losses =1 1=include momentum losses
radioactive_decay =1 1=include radioactive decay
K_capture =1 1=include K-capture
ionization_rate =0 1=compute ionization rate
start_timestep =1.0e9
end_timestep =1.0e2
timestep_factor =0.25
timestep_repeat =20 number of repeats per timestep in timetep_mode=1
timestep_repeat2 =0 number of timesteps in timetep_mode=2
timestep_print =10000 number of timesteps between printings
timestep_diagnostics =10000 number of timesteps between diagnostics
control_diagnostics =0 control detail of diagnostics
network_iterations = 1 number of iterations of entire network
prop_r = 1 1=propagate in r (2D)
prop_x = 1 1=propagate in x (2D,3D)
prop_y = 1 1=propagate in y (3D)
prop_z = 1 1=propagate in z (3D)
prop_p = 1 1=propagate in momentum
use_symmetry = 0 0=no symmetry, 1=optimized symmetry, 2=xyz symmetry by copying(3D)
vectorized = 0 0=unvectorized code, 1=vectorized code
source_specification = 0 2D::1:r,z=0 2:z=0 3D::1:x,y,z=0 2:z=0 3:x=0 4:y=0
source_model = 1 0=zero 1=parameterized 2=Case&B 3=pulsars 4= 5=S&Mattox 6=S&Mattox with cutoff 7=Gaussian
source_parameters_1 = 0.475063 1.25 2.35 model 1:alpha model 7: Gaussian mean, kpc from GC
source_parameters_2 = 2.16570 3.56 5.56283 model 1:beta model 7: Gaussian width, kpc
source_parameters_3 = 15.0 model 1, 7 :rmax: set to zero beyond this radius, kpc from GC
source_parameters_4 = 10.0 model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC
source_parameters_5 = 0.0 not yet used
n_cr_sources = 0 number of pointlike cosmic-ray sources 3D only!
cr_source_x_01 = 10.0 x position of cosmic-ray source 1 (kpc)
cr_source_y_01 = 10.0 y position of cosmic-ray source 1
cr_source_z_01 = 0.1 z position of cosmic-ray source 1
cr_source_w_01 = 0.1 sigma width of cosmic-ray source 1
cr_source_L_01 = 1.0 luminosity of cosmic-ray source 1
cr_source_x_02 = 3.0 x position of cosmic-ray source 2
cr_source_y_02 = 4.0 y position of cosmic-ray source 2
cr_source_z_02 = 0.2 z position of cosmic-ray source 2
cr_source_w_02 = 2.4 sigma width of cosmic-ray source 2
cr_source_L_02 = 2.0 luminosity of cosmic-ray source 2
SNR_events = 0 handle stochastic SNR events
SNR_interval = 1.0e4 time interval in years between SNR in 1 kpc^-3 volume
SNR_livetime = 1.0e4 CR-producing live-time in years of an SNR
SNR_electron_sdg = 0.00 delta electron source index Gaussian sigma
SNR_nuc_sdg = 0.00 delta nucleus source index Gaussian sigma
SNR_electron_dgpivot = 5.0e3 delta electron source index pivot rigidity (MeV)
SNR_nuc_dgpivot = 5.0e3 delta nucleus source index pivot rigidity (MeV)
proton_norm_Ekin = 1.00e+5 proton kinetic energy for normalization (MeV)
proton_norm_flux = 5.00e-9 5.75e-9 6.75e-9 5.75e-9 5.00e-9 to renorm nuclei/flux of protons at norm energy (cm^-2 sr^-1 s^-1 MeV^-1)
electron_norm_Ekin = 3.45e4 electron kinetic energy for normalization (MeV)
electron_norm_flux = 0.32e-9 0.56e-9 0.32e-9 0.4e-9 0.6e-9 0.40e-9 flux of electrons at normalization energy (cm^-2 sr^-1 s^-1 MeV^-1)
max_Z = 8 2 maximum number of nucleus Z listed
use_Z_1 = 1
use_Z_2 = 1
use_Z_3 = 1
use_Z_4 = 1
use_Z_5 = 1
use_Z_6 = 1
use_Z_7 = 1
use_Z_8 = 1
use_Z_9 = 1
use_Z_10 = 1
use_Z_11 = 1
use_Z_12 = 1
use_Z_13 = 1
use_Z_14 = 1
use_Z_15 = 1
use_Z_16 = 1
use_Z_17 = 1
use_Z_18 = 1
use_Z_19 = 1
use_Z_20 = 1
use_Z_21 = 1
use_Z_22 = 1
use_Z_23 = 1
use_Z_24 = 1
use_Z_25 = 1
use_Z_26 = 1
use_Z_27 = 1
use_Z_28 = 1
use_Z_29 = 0
use_Z_30 = 0
iso_abundance_01_001 = 1.06e+06 H
iso_abundance_01_002 = 0. 34.8
iso_abundance_02_003 = 9.033 He
iso_abundance_02_004 = 7.199e+04
iso_abundance_03_006 = 0 Li
iso_abundance_03_007 = 0
iso_abundance_04_009 = 0 Be
iso_abundance_05_010 = 0 B
iso_abundance_05_011 = 0
iso_abundance_06_012 = 2819 C
iso_abundance_06_013 = 5.268e-07
iso_abundance_07_014 = 182.8 N
iso_abundance_07_015 = 5.961e-05
iso_abundance_08_016 = 3822 O
iso_abundance_08_017 = 6.713e-07
iso_abundance_08_018 = 1.286
iso_abundance_09_019 = 2.664e-08 F
iso_abundance_10_020 = 312.5 Ne
iso_abundance_10_021 = 0.003556
iso_abundance_10_022 = 100.1
iso_abundance_11_023 = 22.84 Na
iso_abundance_12_024 = 658.1 Mg
iso_abundance_12_025 = 82.5
iso_abundance_12_026 = 104.7
iso_abundance_13_027 = 76.42 Al
iso_abundance_14_028 = 725.7 Si
iso_abundance_14_029 = 35.02
iso_abundance_14_030 = 24.68
iso_abundance_15_031 = 4.242 P
iso_abundance_16_032 = 89.12 S
iso_abundance_16_033 = 0.3056
iso_abundance_16_034 = 3.417
iso_abundance_16_036 = 0.0004281
iso_abundance_17_035 = 0.7044 Cl
iso_abundance_17_037 = 0.001167
iso_abundance_18_036 = 9.829 Ar
iso_abundance_18_038 = 0.6357
iso_abundance_18_040 = 0.001744
iso_abundance_19_039 = 1.389 K
iso_abundance_19_040 = 3.022
iso_abundance_19_041 = 0.0003339
iso_abundance_20_040 = 51.13 Ca
iso_abundance_20_041 = 1.974
iso_abundance_20_042 = 1.134e-06
iso_abundance_20_043 = 2.117e-06
iso_abundance_20_044 = 9.928e-05
iso_abundance_20_048 = 0.1099
iso_abundance_21_045 = 1.635 Sc
iso_abundance_22_046 = 5.558 Ti
iso_abundance_22_047 = 8.947e-06
iso_abundance_22_048 = 6.05e-07
iso_abundance_22_049 = 5.854e-09
iso_abundance_22_050 = 6.083e-07
iso_abundance_23_050 = 1.818e-05 V
iso_abundance_23_051 = 5.987e-09
iso_abundance_24_050 = 2.873 Cr
iso_abundance_24_052 = 8.065
iso_abundance_24_053 = 0.003014
iso_abundance_24_054 = 0.4173
iso_abundance_25_053 = 6.499 Mn
iso_abundance_25_055 = 1.273
iso_abundance_26_054 = 49.08 Fe
iso_abundance_26_056 = 697.7
iso_abundance_26_057 = 21.67
iso_abundance_26_058 = 3.335
iso_abundance_27_059 = 2.214 Co
iso_abundance_28_058 = 28.88 Ni
iso_abundance_28_060 = 11.9
iso_abundance_28_061 = 0.5992
iso_abundance_28_062 = 1.426
iso_abundance_28_064 = 0.3039
total_cross_section = 2 total cross section option: 0=L83 1=WA96 2=BP01
cross_section_option = 012 100*i+j i=1: use Heinbach-Simon C,O->B j=kopt j=11=Webber, 21=ST
t_half_limit = 1.0e4 year - lower limit on radioactive half-life for explicit inclusion
primary_electrons = 1 1=compute primary electrons
secondary_positrons = 1 1=compute secondary positrons
secondary_electrons = 1 1=compute secondary electrons
knock_on_electrons = 0 1,2 1=compute knock-on electrons (p,He) 2= use factor 1.75 to scale pp,pHe
secondary_antiproton = 0 1,2= calculate: 1=uses nuclear scaling; 2=uses nuclear factors (Simon et al 1998)
tertiary_antiproton = 0 1=compute tertiary antiprotons
secondary_protons = 0 1=compute secondary protons
gamma_rays = 2 2 1=compute gamma rays, 2=compute HI,H2 skymaps separately
pi0_decay = 12 1= old formalism 2=Blattnig et al. 3=Kamae et al. 4=Huang matrices 5=Dermer 6=Kamae 7=Kachelriess 8=Dermer-Kachelriess 9=Kamae-Kachelriess 10=K&O 2013 11=Dermer-Kachelriess2013, 12=Dermer_Kachelriess2013_heavy, 20=FLUKA
IC_isotropic = 1 1,2= compute isotropic IC: 1=compute full, 2=store skymap components
IC_anisotropic = 0 1,2,3= compute anisotropic IC: 1=full, 2=approx., 3=isotropic
synchrotron = 1 1=compute synchrotron
bremss = 1 1=compute bremsstrahlung
comment = the dark matter (DM) switches and user-defined parameters
DM_positrons = 0 1=compute DM positrons
DM_electrons = 0 1=compute DM electrons
DM_antiprotons = 0 1=compute DM antiprotons
DM_gammas = 0 1=compute DM gammas
DM_double0 = 2.8 core radius, kpc
DM_double1 = 0.43 local DM mass density, GeV cm-3
DM_double2 = 80. neutralino mass, GeV
DM_double3 = 40. positron width distribution, GeV
DM_double4 = 40. positron branching
DM_double5 = 40. electron width distribution, GeV
DM_double6 = 30. electron branching
DM_double7 = 50. pbar width distribution, GeV
DM_double8 = 40. pbar branching
DM_double9 =3.e-25 <cross_sec*V>-thermally overaged, cm3 s-1
DM_int0 = 1 isothermal profile
DM_int1 = 1
DM_int2 = 1
DM_int3 = 1
DM_int4 = 1
DM_int5 = 1
DM_int6 = 1
DM_int7 = 1
DM_int7 = 1
DM_int8 = 1
DM_int9 = 1
skymap_format = 3 0 3 fitsfile format: 0=old format (the default), 1=mapcube for glast science tools, 2=both, 3=healpix
output_gcr_full = 1 output full galactic cosmic ray array
warm_start = 0 read in nuclei file and continue run
verbose = 0 -456 -455 -454 -453 verbosity: 0=min,10=max <0: selected debugs
test_suite = 0 run test suite instead of normal run
GALDEF/galdef_54_reltest20 0 → 100644
View file @ 796c27f8
This diff is collapsed.
GALDEF/galdef_55_reltest19 0 → 100644
View file @ 796c27f8
1234567890123456789012
======================value
Title = copy of 55_z04LMo7S but with pion production matrices:pi0_decay=2 QGSJET : 10,11,12 reduced Ekin max, increased E_gamma_min to avoid nan
Title = which was copy of 54_z04LMS with same healpix order 7
Title = which was copy of 54_z02G4c5MS but with Lorimer pulsars (but flat R=10-15 kpc) instead of Gaussian source distribution
Title = which was copy of 54_z10G4c5mS but with B_field =070500030 and wideband gammas and finer sync.all compatible with z02,z04*MS Ekin_min=100 MeV 10 per decade CR and gamma
Title = which was copy of 54_z10G4c5kS but no flattening of Gaussian source in outer Galaxy
Title = which was copy of 54_z10G4c5rS but galprop r381 new CO analytical model, EBV: 2mag cut, no b cut
Title = which was copy of 54_z10FenprS but with Gaussian source, 4.5 kpc flat beyond 8.5 kpc
Title = which was copy of 54_z04FenprS but zh=10 and appropriate Dxx
Title = which was copy of 54_z04FenpDS but with new CO, type 3 ISRF. Reference models for paper 2.
Title = which was copy of 54_z04FelD7S but with Fermi electrons unscaled, protons unscaled, Gaensler HII. B_field and gas model parameters added
Title = which was copy of 54_z04Feld7S but with E(B-V) local HI ring with pos and neg residuals, bmin=5, E(B-V) max =5
Title = which was copy of 54_z04Felh7S but with E(B-V) local HI ring as in z04epmdGS
Title = which was copy of 54_87Xexph7S but with Fermi electrons unscaled, protons*1.15. galprop r275
Title = which was copy of 54_86Xexph7S but with energy range 50 MeV - 100 GeV, 30 bins as requested by Seth. integration mode changed to 0 to avoid bremss wiggles
Title = which was copy of 54_85Xexph7S but with protons factor 1.35 instead of 1.30
Title = which was copy of 54_82Xexph7S but with protons factor 1.30 instead of 1.15
Title = which was copy of 54_81Xexph7S but with moment-masked CO dataset
Title = which was copy of 54_77Xexph7S but with CR gradient adjusted to give more in outer Galaxy see Fermi paper 2 gradplot.pro
Title = which was copy of 54_77Xvarh7S but with exponential Xco based on recent Fermi results: 10^(-0.4+0.066*R)
Title = which was copy of 54_72Xvarh7S but with new CO map from Gulli rbands_co9 and galprop r223 with reinstated store_IC_skymap
Title = which was copy of 54_71Xvarh7S but with p,He and electrons scaled based on gardian all-sky fit, p,He factor=1.15, electrons factor=1.75
Title = which was copy of 54_70Xvarh7S but with electron injection spectrum 2.42
Title = which was copy of 54_5FXvarh7S but with electron injection adjusted to Fermi
Title = which was copy of 54_5EXvarh7S but with Kamae pion-decay instead of old formalism
Title = which was copy of 54_5BXvarh7S but with electrons factor 0.4e-9 instead of 0.6e-9 (i.e. original conventional model)
Title = which was copy of 54_5Avarh7S but with higher gamma-ray energy resolution
Title = which was copy of 54_56varh7S but with new gradient and electrons *1.5 from gardian 4-ring fit using dubois to 22 Aug
Title = which was copy of 54_55Xvarh7S but with Ekin_max=1.0e9
Title = which was copy of 54_610202h7S but n_X_CO=9 for standard variation of X_CO and source under v54, propagation parameters from galdef_53_5102229RG
Title = with e+e- secondaries and smaller E_gamma_factor than 54_54Xvarh7S
n_spatial_dimensions = 2
r_min =00.0 min r
r_max =20.00 max r
dr = 1.0 delta r
z_min =-04.0 min z
z_max =+04.0 max z
dz = 0.1 delta z
x_min =-10.0 min x
x_max =+10.0 max x
dx = 1.0 delta x
y_min =-10.0 min y
y_max =+10.0 max y
dy = 1.0 delta y
p_min =1000 min momentum (MV)
p_max =4000 max momentum
p_factor =1.50 momentum factor
Ekin_min =1.0e2 min kinetic energy per nucleon (MeV)
Ekin_max =1.0e8 1.0e9 max kinetic energy per nucleon 1e9 gives nan or inf for pi0 method 10
Ekin_factor =1.2589254 1.2 kinetic energy per nucleon factor
p_Ekin_grid = Ekin p||Ekin alignment
E_gamma_min = 1.0e-2 1.0 1.0e-2 min gamma-ray energy (MeV) 1e-2 gives nan for pi0 method 10
E_gamma_max = 1.0e+7 max gamma-ray energy (MeV)
E_gamma_factor = 1.2589254 1.2996566 gamma-ray energy factor
integration_mode = 0 integr.over part.spec.: =1-old E*logE; =0-PL analyt.
nu_synch_min = 1.0e6 min synchrotron frequency (Hz)
nu_synch_max = 1.0e12 max synchrotron frequency (Hz)
nu_synch_factor = 1.1 synchrotron frequency factor
long_min = 0.25 gamma-ray intensity skymap longitude minimum (deg); 0 -automatic binning required to get correct results!
long_max =359.75 gamma-ray intensity skymap longitude maximum (deg); 360 -automatic binning
lat_min =-89.75 gamma-ray intensity skymap latitude minimum (deg); -90 -automatic binning
lat_max =+89.75 gamma-ray intensity skymap latitude maximum (deg); +90 -automatic binning
d_long = 0.5 gamma-ray intensity skymap longitude binsize (deg)
d_lat = 0.5 gamma-ray intensity skymap latitude binsize (deg)
healpix_order = 7 order for healpix skymaps. 7 gives ~0.5 deg and it changes by an order of 2
lat_substep_number = 1 latitude bin splitting (0,1=no split, 2=split in 2...)
LoS_step = 0.01 kpc, Line of Sight (LoS) integration step
LoS_substep_number = 1 number of substeps per LoS integration step (0,1=no substeps)
D0_xx = 5.8e28 diffusion coefficient at reference rigidity
D_rigid_br =4.0e3 reference rigidity for diffusion coefficient in MV
D_g_1 = 0.33 diffusion coefficient index below reference rigidity
D_g_2 = 0.33 diffusion coefficient index above reference rigidity
diff_reacc =1 0=no reacc.; 1,2=incl.diff.reacc.; -1==beta^3 Dxx; 11=Kolmogorov+damping; 12=Kraichnan+damping
v_Alfven =30. Alfven speed in km s-1
damping_p0 = 1.e6 MV -some rigidity (where CR density is low)
damping_const_G = 0.02 a const derived from fitting B/C
damping_max_path_L = 3.e21 Lmax~1 kpc, max free path
convection =0 1=include convection
v0_conv =0. km s-1 v_conv=v0_conv+dvdz_conv*dz
dvdz_conv =10. km s-1 kpc-1 v_conv=v0_conv+dvdz_conv*dz
nuc_rigid_br = 9.0e3 reference rigidity for nucleus injection index in MV
nuc_g_1 =1.98 nucleus injection index below reference rigidity
nuc_g_2 =2.42 nucleus injection index index above reference rigidity
inj_spectrum_type = rigidity rigidity||beta_rig||Etot nucleon injection spectrum type
electron_g_0 =1.60 electron injection index below electron_rigid_br0
electron_rigid_br0 =4.0e3 reference rigidity0 for electron injection index in MV
electron_g_1 =2.42 2.3 2.54 electron injection index below reference rigidity
electron_rigid_br =1.0e9 reference rigidity for electron injection index in MV
electron_g_2 =5.0 electron injection index index above reference rigidity
He_H_ratio = 0.11 He/H of ISM, by number
n_X_CO = 10 an option to select functional dependence of X_CO=X_CO(R) 0=constant as below, 9=standard variation as in A&A 2004 paper 10=an exponential
X_CO = 1.9E20 conversion factor from CO integrated temperature to H2 column density
nHI_model = 1 selection of HI gas density model (not yet implemented)
nH2_model = 1 selection of H2 gas density model (not yet implemented)
nHII_model = 3 selection of HII gas density model 1=Cordes et al 1991 2=NE2001 3 = Gaensler etal 2008
COR_filename = rbands_co10mm_v2_2001_qdeg.fits.gz rbands_co10mm_2001_qdeg.fits.gz rbands_co9_qdeg.fits.gz
HIR_filename = rbands_hi12_v2_qdeg_zmax1_Ts125_EBV2.0_localring_4.fits rbands_hi12_v2_qdeg_zmax1_Ts125_EBV_localring_3.fits rbands_hi12_qdeg_zmax1.fits.gz
B_field_model = 070500030 bbbrrrzzz bbb=10*B(0) rrr=10*rscale zzz=10*zscale
B_field_name = galprop_original han_ran 3D models:han .... galprop_original: exponential model as in original (parameters Bo, rscale, zscale)
n_B_field_parameters = 10 number of B-field parameters (must be 10 at present)
B_field_parameters = 9.0e-6,65.0,-8.5,12.26,5.00e-6,0.0,0.0,0.0,0.0,0.2 parameters for 3D models, meaning depends on the model
ISRF_file = ISRF/Standard/Standard.dat ISRF_RMax20_ZMax5_DR0.5_DZ0.1_MW_BB_24092007.fits input ISRF file
ISRF_filetype = 3 2 3=new 2=old NB this changed from 1 to 2 for the same file type
ISRF_healpixOrder = 3 for output of ISRF skymaps
ISRF_factors = 1.0,1.0,1.0 ISRF factors for IC calculation: optical, FIR, CMB
fragmentation =1 1=include fragmentation
momentum_losses =1 1=include momentum losses
radioactive_decay =1 1=include radioactive decay
K_capture =1 1=include K-capture
ionization_rate =0 1=compute ionization rate
start_timestep =1.0e9
end_timestep =1.0e2
timestep_factor =0.25
timestep_repeat =20 number of repeats per timestep in timetep_mode=1
timestep_repeat2 =0 number of timesteps in timetep_mode=2
timestep_print =10000 number of timesteps between printings
timestep_diagnostics =10000 number of timesteps between diagnostics
control_diagnostics =0 control detail of diagnostics
network_iterations = 1 number of iterations of entire network
prop_r = 1 1=propagate in r (2D)
prop_x = 1 1=propagate in x (2D,3D)
prop_y = 1 1=propagate in y (3D)
prop_z = 1 1=propagate in z (3D)
prop_p = 1 1=propagate in momentum
use_symmetry = 0 0=no symmetry, 1=optimized symmetry, 2=xyz symmetry by copying(3D)
vectorized = 0 0=unvectorized code, 1=vectorized code
source_specification = 0 2D::1:r,z=0 2:z=0 3D::1:x,y,z=0 2:z=0 3:x=0 4:y=0
source_model = 1 0=zero 1=parameterized 2=Case&B 3=pulsars 4= 5=S&Mattox 6=S&Mattox with cutoff 7=Gaussian
source_parameters_1 = 0.475063 1.25 2.35 model 1:alpha model 7: Gaussian mean, kpc from GC
source_parameters_2 = 2.16570 3.56 5.56283 model 1:beta model 7: Gaussian width, kpc
source_parameters_3 = 15.0 model 1, 7 :rmax: set to zero beyond this radius, kpc from GC
source_parameters_4 = 10.0 model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC
source_parameters_5 = 0.0 not yet used
n_cr_sources = 0 number of pointlike cosmic-ray sources 3D only!
cr_source_x_01 = 10.0 x position of cosmic-ray source 1 (kpc)
cr_source_y_01 = 10.0 y position of cosmic-ray source 1
cr_source_z_01 = 0.1 z position of cosmic-ray source 1
cr_source_w_01 = 0.1 sigma width of cosmic-ray source 1
cr_source_L_01 = 1.0 luminosity of cosmic-ray source 1
cr_source_x_02 = 3.0 x position of cosmic-ray source 2
cr_source_y_02 = 4.0 y position of cosmic-ray source 2
cr_source_z_02 = 0.2 z position of cosmic-ray source 2
cr_source_w_02 = 2.4 sigma width of cosmic-ray source 2
cr_source_L_02 = 2.0 luminosity of cosmic-ray source 2
SNR_events = 0 handle stochastic SNR events
SNR_interval = 1.0e4 time interval in years between SNR in 1 kpc^-3 volume
SNR_livetime = 1.0e4 CR-producing live-time in years of an SNR
SNR_electron_sdg = 0.00 delta electron source index Gaussian sigma
SNR_nuc_sdg = 0.00 delta nucleus source index Gaussian sigma
SNR_electron_dgpivot = 5.0e3 delta electron source index pivot rigidity (MeV)
SNR_nuc_dgpivot = 5.0e3 delta nucleus source index pivot rigidity (MeV)
proton_norm_Ekin = 1.00e+5 proton kinetic energy for normalization (MeV)
proton_norm_flux = 5.00e-9 5.75e-9 6.75e-9 5.75e-9 5.00e-9 to renorm nuclei/flux of protons at norm energy (cm^-2 sr^-1 s^-1 MeV^-1)
electron_norm_Ekin = 3.45e4 electron kinetic energy for normalization (MeV)
electron_norm_flux = 0.32e-9 0.56e-9 0.32e-9 0.4e-9 0.6e-9 0.40e-9 flux of electrons at normalization energy (cm^-2 sr^-1 s^-1 MeV^-1)
max_Z = 8 2 maximum number of nucleus Z listed
use_Z_1 = 1
use_Z_2 = 1
use_Z_3 = 1
use_Z_4 = 1
use_Z_5 = 1
use_Z_6 = 1
use_Z_7 = 1
use_Z_8 = 1
use_Z_9 = 1
use_Z_10 = 1
use_Z_11 = 1
use_Z_12 = 1
use_Z_13 = 1
use_Z_14 = 1
use_Z_15 = 1
use_Z_16 = 1
use_Z_17 = 1
use_Z_18 = 1
use_Z_19 = 1
use_Z_20 = 1
use_Z_21 = 1
use_Z_22 = 1
use_Z_23 = 1
use_Z_24 = 1
use_Z_25 = 1
use_Z_26 = 1
use_Z_27 = 1
use_Z_28 = 1
use_Z_29 = 0
use_Z_30 = 0
iso_abundance_01_001 = 1.06e+06 H
iso_abundance_01_002 = 0. 34.8
iso_abundance_02_003 = 9.033 He
iso_abundance_02_004 = 7.199e+04
iso_abundance_03_006 = 0 Li
iso_abundance_03_007 = 0
iso_abundance_04_009 = 0 Be
iso_abundance_05_010 = 0 B
iso_abundance_05_011 = 0
iso_abundance_06_012 = 2819 C
iso_abundance_06_013 = 5.268e-07
iso_abundance_07_014 = 182.8 N
iso_abundance_07_015 = 5.961e-05
iso_abundance_08_016 = 3822 O
iso_abundance_08_017 = 6.713e-07
iso_abundance_08_018 = 1.286
iso_abundance_09_019 = 2.664e-08 F
iso_abundance_10_020 = 312.5 Ne
iso_abundance_10_021 = 0.003556
iso_abundance_10_022 = 100.1
iso_abundance_11_023 = 22.84 Na
iso_abundance_12_024 = 658.1 Mg
iso_abundance_12_025 = 82.5
iso_abundance_12_026 = 104.7
iso_abundance_13_027 = 76.42 Al
iso_abundance_14_028 = 725.7 Si
iso_abundance_14_029 = 35.02
iso_abundance_14_030 = 24.68
iso_abundance_15_031 = 4.242 P
iso_abundance_16_032 = 89.12 S
iso_abundance_16_033 = 0.3056
iso_abundance_16_034 = 3.417
iso_abundance_16_036 = 0.0004281
iso_abundance_17_035 = 0.7044 Cl
iso_abundance_17_037 = 0.001167
iso_abundance_18_036 = 9.829 Ar
iso_abundance_18_038 = 0.6357
iso_abundance_18_040 = 0.001744
iso_abundance_19_039 = 1.389 K
iso_abundance_19_040 = 3.022
iso_abundance_19_041 = 0.0003339
iso_abundance_20_040 = 51.13 Ca
iso_abundance_20_041 = 1.974
iso_abundance_20_042 = 1.134e-06
iso_abundance_20_043 = 2.117e-06
iso_abundance_20_044 = 9.928e-05
iso_abundance_20_048 = 0.1099
iso_abundance_21_045 = 1.635 Sc
iso_abundance_22_046 = 5.558 Ti
iso_abundance_22_047 = 8.947e-06
iso_abundance_22_048 = 6.05e-07
iso_abundance_22_049 = 5.854e-09
iso_abundance_22_050 = 6.083e-07
iso_abundance_23_050 = 1.818e-05 V
iso_abundance_23_051 = 5.987e-09
iso_abundance_24_050 = 2.873 Cr
iso_abundance_24_052 = 8.065
iso_abundance_24_053 = 0.003014
iso_abundance_24_054 = 0.4173
iso_abundance_25_053 = 6.499 Mn
iso_abundance_25_055 = 1.273
iso_abundance_26_054 = 49.08 Fe
iso_abundance_26_056 = 697.7
iso_abundance_26_057 = 21.67
iso_abundance_26_058 = 3.335
iso_abundance_27_059 = 2.214 Co
iso_abundance_28_058 = 28.88 Ni
iso_abundance_28_060 = 11.9
iso_abundance_28_061 = 0.5992
iso_abundance_28_062 = 1.426
iso_abundance_28_064 = 0.3039
total_cross_section = 2 total cross section option: 0=L83 1=WA96 2=BP01
cross_section_option = 012 100*i+j i=1: use Heinbach-Simon C,O->B j=kopt j=11=Webber, 21=ST
t_half_limit = 1.0e4 year - lower limit on radioactive half-life for explicit inclusion
primary_electrons = 1 1=compute primary electrons
secondary_positrons = 1 1=compute secondary positrons
secondary_electrons = 1 1=compute secondary electrons
knock_on_electrons = 0 1,2 1=compute knock-on electrons (p,He) 2= use factor 1.75 to scale pp,pHe
secondary_antiproton = 0 1,2= calculate: 1=uses nuclear scaling; 2=uses nuclear factors (Simon et al 1998)
tertiary_antiproton = 0 1=compute tertiary antiprotons
secondary_protons = 0 1=compute secondary protons
gamma_rays = 2 2 1=compute gamma rays, 2=compute HI,H2 skymaps separately
pi0_decay = 12 1= old formalism 2=Blattnig et al. 3=Kamae et al. 4=Huang matrices 5=Dermer 6=Kamae 7=Kachelriess 8=Dermer-Kachelriess 9=Kamae-Kachelriess 10=K&O 2013 11=Dermer-Kachelriess2013, 12=Dermer_Kachelriess2013_heavy, 20=FLUKA
IC_isotropic = 1 1,2= compute isotropic IC: 1=compute full, 2=store skymap components
IC_anisotropic = 0 1,2,3= compute anisotropic IC: 1=full, 2=approx., 3=isotropic
synchrotron = 1 1=compute synchrotron
bremss = 1 1=compute bremsstrahlung
comment = the dark matter (DM) switches and user-defined parameters
DM_positrons = 0 1=compute DM positrons
DM_electrons = 0 1=compute DM electrons
DM_antiprotons = 0 1=compute DM antiprotons
DM_gammas = 0 1=compute DM gammas
DM_double0 = 2.8 core radius, kpc
DM_double1 = 0.43 local DM mass density, GeV cm-3
DM_double2 = 80. neutralino mass, GeV