https://github.com/a-e-egorov/GALPROP_DM
Tip revision: 3e42307006508424bc7beadd0708f6c240029339 authored by Andrei Egorov on 02 February 2024, 16:17:56 UTC
Update DM-v57_w_M31.patch
Update DM-v57_w_M31.patch
Tip revision: 3e42307
galdef_56_testM31MED
#Title = example of DM run for M31 for MED DM density, MF and prop. parameters
# DARK MATTER and other var =====================================================
DM_double2 = 100 DM particle mass, GeV - must be in [5..100000] AND > rest mass of the primary products (DM_int2)
DM_double9 = 2e-26 DM thermally averaged annihilation cross section, cm^3 s^-1
DM_int2 = 6 DM annihilation channel: 1=e^+e^-, 2=\mu^+\mu^-,3=\tau^+\tau^-,4=qq*, 5=cc*, 6=bb*, 7=tt*, 8=\gamma\gamma, 9=gg, 10=W^+W^-, 11=ZZ, 12=hh
DM_int0 = 0 DM density profile (according to PPPC): 0=generalized NFW, 1=Isothermal, 2=Einasto, 3=Burkert, 9=DarkSUSY
DM_double6 = 1.0 \gamma parameter for the generalized NFW profile (1.0 gives the canonical NFW)
DM_double1 = 0.585 scale density of the DM profile, GeV cm^-3
DM_double0 = 10.4 scale radius of the DM density profile, kpc
DM_double8 = 0.01 truncation radius for the NFW profile, below which the DM density stays constant, kpc (must be >0!)
DM_double7 = 0.73 \alpha parameter for the Einasto DM density profile
DM_int3 = 0 Substructure presense: 0=no, 1=based on Kamionkowski et al., Phys.Rev.D 81, 043532 (2010).
ISRF_factors = 2.0,0.1,1.0 ISRF factors for IC calculation: optical, FIR, CMB
DM_int9 = 8 0=fixed increment synchrotron frequency grid, >0=# of arbitrary frequencies (DM_double3)
DM_double3 = 0.074e9,0.147e9,0.34e9,1.5e9,2.6e9,4.9e9,6.6e9,8.4e9 list of arbitrary synchrotron frequencies (Hz)
cameraLocation = 48.0631,0,13.7819 33.6,0,9.65 #Specifies the camera location in x,y,z. Sun is at positive x.
healpix_order = 10 #order for healpix skymaps. 7 gives ~0.5 deg and it changes by an order of 2
DM_double4 = 0.03 central electrons' density in cm^-3
HII_Te = 7000 free electron temperature (K) for free-free absorption
HII_clumping_factor = 21 free electron clumping factor for free-free absorption
DM_int4 = 1 1=doubles lepton source function (0=no) in order to save comp. time by propagating only one specie; if turned on, requires either one of DM_positrons or DM_electrons to be 0; should be a good approximation
DM_positrons = 0 1=compute DM positrons
DM_electrons = 1 1=compute DM electrons
DM_antiprotons = 0 1=compute DM antiprotons
DM_gammas = 0 1=compute DM gammas
DM_int8 = 1 not used
DM_int5 = 1
DM_int6 = 1
DM_int7 = 1
DM_int1 = 1 9=DarkSUSY DM source
DM_double5 = 40.
gamma_rays = 0 1=compute gamma rays, 2=compute HI,H2 skymaps separately
pi0_decay = 0 1= old formalism 2=Blattnig et al. 3=Kamae et al.
IC_isotropic = 0 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
bremss = 0 1=compute bremsstrahlung
synchrotron = 2 2,3=compute synchrotron using B_field_model and B_field_parameters. 2=total only, 3=all Stokes
free_free_absorption = 1 0= no absorption 1= free-free absorption
# MAGNETIC FIELD ================================================
B_field_name = M31-MED 3D models:han ..galprop_original: exponential model as in original (parameters Bo, rscale, zscale)
# B0 R- z-scale
B_field_parameters = 6.0e-6, 4.0, 1.2 , 0.0,0.0,0.0,0.0,0.0,0.0,0.0 parameters for 3D models galprop_original
# PROPAGATION ===================================================
z_min = -2.7 min z, kpc
z_max = +2.7 max z, kpc
D0_xx = 6e27 diffusion coefficient in x at reference rigidity in cm^2/s
D_g_1 = 0.45 diffusion coefficient index below reference rigidity
D_g_2 = 0.45 diffusion coefficient index above reference rigidity
D_rigid_ref = 1.0e3 #Reference rigidity for normalization
D_rigid_br = 1.0e3 reference rigidity for diffusion coefficient in MV
D_eta = -2 #Exponent on the beta multiplication for D0_xx, defaults to 1
diff_reacc = 0 0=no reacc.; 1,2=incl.diff.reacc.; -1==beta^3 Dxx; 11=Kolmogorov+damping; 12=Kraichnan+damping
v_Alfven = 5.0 Alfven speed in km s^-1
#Spatially dependent diffusion
B_dep_diffusion =0 #Link D0_xx and v_Alfven to the magnetic field model
D_xx_max =1e30 #Maximum diffusion coefficient at 10 GV, used when B_dep_diffusion = 1
D_xx_min =1e26 #Minimum diffusion coefficient at 10 GV, used when B_dep_diffusion = 1
#Reduction of diffusion in the plane
Dxx_plane_scale =-1 #Multiply the Dxx value in the plane with this value. Ignored if negative
Dxx_plane_scale_height =0.2 #Scale height for the normalization
#Used in damping only
#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_const_K = 0.1 #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
output_gcr_full = 0 #output full galactic cosmic ray array
# ================================================================
n_spatial_dimensions = 2
dz = 0.05 delta z, kpc
dr = 0.05 delta r
r_min = 0.0 min r
r_max = 15 max r
x_min = -15 min x
x_max = +15 max x
dx = 0.2 delta x
y_min = -15 min y
y_max = +15 max y
dy = 0.2 delta y
p_Ekin_grid = Ekin p||Ekin alignment
#p_min = 1000 min momentum (MV)
#p_max = 4000 max momentum
#p_factor = 1.50 momentum factor
Ekin_min = 10 min kinetic energy per nucleon (MeV); not only the region of interest must be covered, but also the region of production
Ekin_max = 1.2e5 max kinetic energy per nucleon (MeV); not only the region of interest must be covered, but also the region of production
Ekin_factor = 1.04 kinetic energy per nucleon grid factor
E_gamma_min = 1. min gamma-ray energy (MeV)
E_gamma_max = 1000. max gamma-ray energy (MeV)
E_gamma_factor = 3.0 gamma-ray energy factor
integration_mode = 0 integr.over part.spec.: =1-old E*logE; =0-PL analyt. (0 is recommended)
nu_synch_min = 28.0e9 min synchrotron frequency (Hz)
nu_synch_max = 29.0e9 max synchrotron frequency (Hz)
nu_synch_factor = 1.5 synchrotron frequency factor
skymap_format = 3 #fitsfile format: 0=old format (the default), 1=mapcube for glast science tools, 2=both, 3=healpix
anisoHealpixOrder = 1 #Specifies the order in which to calculate the aniso/iso IC calculation. This map is then interpolated to the output order
#Specify los integration mode
los_integration_mode = 1 #0 - old fixed step size code without interpolation in all but IC
#1 - new code with variable step size and interpolation.
LoS_step = 0.01 #kpc, Line of Sight (LoS) integration step for mode 0, inital step for mode 1
#This should be a small number for improved accuracy and stability of los_integration_mode 1
#Following options only for los_integration_mode 0
lat_substep_number = 1 #latitude bin splitting (0,1=no split, 2=split in 2...)
LoS_substep_number = 1 #number of substeps per LoS integration step (0,1=no substeps)
#This option only for los_integration_mode 1
los_integration_accuracy = 1e-3 #Relative accuracy for the integration
LoS_minStep = 1e-4 # Minimum step size
He_H_ratio = 0.1 He/H of ISM, by number
n_X_CO = 9 #an option to select functional dependence of X_CO=X_CO(R)
#0=constant as below,
#1=tabulated values with linear interpolation using X_CO_radius and X_CO_values
#2=exponential function with a constant and a linear term X_CO = X0 + X1*r + X2*10**(X3*r). Xi retrieved from X_CO_parameters below
#3=tabulated values with power-law interpolation using X_CO_radius and X_CO_values
#9=standard variation as in A&A 2004 paper
#10=an exponential function X_CO = 1e20 * 10**(a + b*r) with a = -0.4 and b = 0.066. Fixed above r=15kpc
X_CO = 1.9E20 conversion factor from CO integrated temperature to H2 column density, n_X_CO = 0 only
X_CO_parameters = 1e20, 1.5, 0.1, 5e-2 #comma separated list of values for n_X_CO = 2
#Tabulated values for n_X_CO = 1 and 3. Should be same size
#X_CO_values = 1e19, 1e20, 2e20, 1e20, 5e20
#X_CO_radius = 0, 3, 5, 9, 20 #in kpc
nHI_model = 4 #selection of HI gas density model 1=old incorrect model, 2=standard model, 9=XML model
nH2_model = 4 #selection of H2 gas density model 1=old incorrect model, 2=standard model, 9=XML model
nHII_model = 4 #selection of HII gas density model 1=Cordes et al 1991 2, 3 = other models, 9=XML model
HI_xmlFilename = path #path to a xml file that describes the HI gas model using libgalstruct
H2_xmlFilename = path #path to a xml file that describes the CO gas model using libgalstruct
HII_xmlFilename = path #path to a xml file that describes the HII gas model using libgalstruct
#The annuli are only used for gamma-ray output
COR_filename = #rbands_co10mm_v3_2001_hdeg.fits.gz #CO gas annuli, not used if empty
HIR_filename = #rbands_hi12_v5_hdeg_zmax1_Ts125.fits.gz #HI gas annuli, not used if empty
#ISRF, used in both energy losses and Inverse Compton calculation
ISRF_file = FITS/ISRF/Standard/Standard.dat #input ISRF file THIS IS THE ONE FOR ANISOTROPIC IC
ISRF_filetype = 3 0=CMB only,1=obsolete, 2=standard FITS, 3=healpix with angular dependence
ISRF_healpixOrder = 3 #for aniso IC calculation, specifies the IRFS skymap order
fragmentation = 0 1=include fragmentation
momentum_losses = 1 1=include momentum losses
radioactive_decay = 0 1=include radioactive decay
K_capture = 0 1=include K-capture
ionization_rate = 0 1=compute ionization rate
ionization_losses = 1 #To turn off ionization energy losses
coulomb_losses = 1 #To turn off coulomb energy losses
bremss_losses = 1 #To turn off bremsstrahlung energy losses
IC_losses = 1 #To turn off inverse Compton energy losses
sync_losses = 1 #To turn off synchrotron energy losses
primary_electrons = 0 1=compute primary electrons
primary_positrons = 0 1=compute primary positrons
secondary_electrons = 0 1=compute secondary electrons
secondary_positrons = 0 1=compute secondary positrons
knock_on_electrons = 0 1,2 1=compute knock-on electrons (p,He) 2= use factor 1.75 to scale pp,pHe
pairproduction = 0 1=compute pair production on ISRF and also absorption if los_integration_mode = 1
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
globalLuminosities = 0 1=compute global luminosities, 0=don't (default)
# Solution settings
start_timestep = 2.0e8
end_timestep = 1.0e1
timestep_factor = 0.5
timestep_repeat = 100 number of repeats per timestep in timetep_mode=1 - must be integer! - this set gives about 2500 steps in total
timestep_repeat2 = 0 number of timesteps in timetep_mode=2
timestep_print = 1000000000 number of timesteps between printings
timestep_diagnostics = 100 number of timesteps between diagnostics
control_diagnostics = 0 control detail of diagnostics
solution_method = 1 1 Crank-Nicolson, 2,21: fully explicit in time, 4 vectorized Crank-Nicolson
solution_convergence = 1 1=use convergence test
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
#----------------------
# CR source distribution
#
# There is a new way to specify the CR source distribution that allows for many
# different source distributions in a single galprop run. The distributions are
# configured in their own configuration files that are then specified with the
# following option. The code looks for the files in the current directory and
# the GALDEF directory. Full paths are also accepted. Many files can be added.
#
# Relative normalization between the different source classes is important.
# Primary positron sources are normalized with electrons, everything else is
# normalized with the protons.
# If this variable is empty we use the options described below to specify the CR
# source distribution.
#source_class_files = exampleSourceClass.txt
#Old options used only if source_class_files is empty
## ---- Start old values ----
source_normalization = 1 #Normalization parameter to control the nuclei flux if proton_norm_flux is 0
electron_source_normalization = 1 #Normalization parameter to control the electron flux if electron_norm_flux is 0
#Should be 0. other values limit the distribution in various ways.
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
#Which distribution type to use. 1 is the most common.
source_model = 1 #0=zero
#1=parameterized f(r) = ((r+sp5)/(rsun+sp5))**sp1 * exp(-sp2*(r-rsun)/(rsun+sp5)), 0 for r > sp3, constant for r > sp4
#2=Case&B
#3=pulsars
#5=S&Mattox
#6=S&Mattox with cutoff
#7=Gaussian sp1 is mean of Gaussian in kcp, sp2 is sigma of gaussian. 0 for r > sp3, constant for r > sp4
#8=Tabulated values from source_values and source_radius
#9=Use total gas distribution nHI + 2nH2
#10=Use H2 gas distribution only
#11=Use HII gas distribution
#12=NE2001 distribution with arms and GC component
#13= bulge + thin disk from ISRF
#14=model 1 + ellipsoid centred on GC
#15=read in the model from an libgalstruct compatible XML file
source_parameters_0 = 0.2 #Gives zscale for models 1 through 8; disc density for 13 and bulge density for 14
source_parameters_1 = 0.475063 #model 1:alpha model 7: Gaussian mean, kpc from GC, model 13: disc R scale, model 14: bulgeA
source_parameters_2 = 2.16570 #model 1:beta model 7: Gaussian width, kpc, model 13: disc Z scale, model 14: bulgeB
source_parameters_3 = 15.0 #model 1, 7 :rmax: set to zero beyond this radius, kpc from GC, model 13: bulge density, model 14: bulgeScaleLength
source_parameters_4 = 10.0 #model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC, model 13: bulgeA, model 14: alpha
source_parameters_5 = 0.0 #model 1: offset for function, model 13: bulgeB, model 14: beta
source_parameters_6 = 0.0 #model 13: bulgeScaleLength, model 14: rmax
source_parameters_7 = 0.0 #model 13: bulgeIndex, model 14: rconst
source_parameters_8 = 0.0 #model 13: phiOffset in degrees, model 14: roff
source_parameters_9 = 0.0 #model 14: zscale
#Electrons can have a different distribution. Defaults to the source_model if not specified.
source_model_elec = 1 #source model for electrons (parameter values default to nuclei values if they are absent), please see documentation above
source_pars_elec_0 = 0.2 #Gives zscale for models 1 through 8; disc density for 13 and bulge density for 14
source_pars_elec_1 = 0.475063 #model 1:alpha model 7: Gaussian mean, kpc from GC, model 13: disc R scale, model 14: bulgeA
source_pars_elec_2 = 2.16570 #model 1:beta model 7: Gaussian width, kpc, model 13: disc Z scale, model 14: bulgeB
source_pars_elec_3 = 15.0 #model 1, 7 :rmax: set to zero beyond this radius, kpc from GC, model 13: bulge density, model 14: bulgeScaleLength
source_pars_elec_4 = 10.0 #model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC, model 13: bulgeA, model 14: alpha
source_pars_elec_5 = 0.0 #model 1: offset for function, model 13: bulgeB, model 14: beta
source_pars_elec_6 = 0.0 #model 13: bulgeScaleLength, model 14: rmax
source_pars_elec_7 = 0.0 #model 13: bulgeIndex, model 14: rconst
source_pars_elec_8 = 0.0 #model 13: phiOffset in degrees, model 14: roff
source_pars_elec_9 = 0.0 #model 14: zscale
#source_xmlFile = path #Only for model 15
#Linear interpolation between values.
#source_radius = 0,1,2,3,4,5,6,7,8,9,10,20 #model 8: radius for points for CR source distribution, kpc from GC
#source_values = 2,3,4,5,6,7,6,5,4,3,02,01 #model 8: values at points for CR source distribution
#source_radius_electrons = 0,1,2,3,4,5,6,7,8,9,10,20 #model 8: radius for points for CR source distribution, kpc from GC
#source_values_electrons = 2,3,4,5,6,7,6,5,4,3,02,01 #model 8: values at points for CR source distribution
#CR point sources, not really tested.
#We need the same number of cr_source_?_i as there are sources and the format of i has to be %02d (two numbers, zero padded below 10)
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
#Even less tested.
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)
#Local bubble, multplies the gas and/or CR source distribution in a radius around the Sun
local_bubble_radius = 0
local_bubble_gas_fraction = 1.0
local_bubble_source_fraction = 1.0
#---------------------
#---------------------
# Injection spectra
inj_spectrum_type = rigidity #rigidity||beta_rig||Etot||dirac||step||expcutoff||doubleexpcutoff nucleon injection spectrum type
#Limit the source injection spectrum range. Not the same as changing the propagation boundaries. All limits are applied if specified so best to specify either rigidity or injection limit.
#rigid_min = 0 #Lower boundary for source injection spectrum in rigidity. Defaults to 0
#rigid_max = 1e31 #Upper boundary for source injcetion spectrum in rigidity. Automatically assigned to maximum double value.
#inj_Ekin_min = 0 #Lower boundary for source injection spectrum in kinetic energy. Defaults to 0
#inj_Ekin_max = 1e31 #Upper boundary for source injcetion spectrum in kinetic energy. Automatically assigned to maximum double value.
#Default double broken power-law for nuclei, used when type is rigidity
nuc_rigid_br0 = 10.0e3
nuc_rigid_br = 220e3 #reference rigidity for nucleus injection index in MV
nuc_g_0 = 1.9 #nucleus injection index index below nuc_rigid_br0
nuc_g_1 = 2.4 #nucleus injection index between rigidity breaks
nuc_g_2 = 2.3 #nucleus injection index index above nuc_rigid_br
#Injection spectrum can be modified for each isotope using
#nuc_rigid_br0_ZZ_AAA = 5e3
#nuc_rigid_br_ZZ_AAA = 200e3
#nuc_g_0_ZZ_AAA = 1.8
#nuc_g_1_ZZ_AAA = 2.3
#nuc_g_2_ZZ_AAA = 2.2
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 #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
#----------------------------
# Normalization for nuclei and electrons
#Galprop normalizes the spectrum post-propagation to these values at the solar location.
#All species, apart from Positrons and Electrons are normalized with respect to protons.
#Use the isotopic abundances to set the relative normalization between elements
proton_norm_Ekin = 1.00e+5 #proton kinetic energy for normalization (MeV)
proton_norm_flux = 0 #to renorm nuclei/flux of protons at norm energy (cm^-2 sr^-1 s^-1 MeV^-1), 0 turns off normalization
electron_norm_Ekin = 3.45e4 #electron kinetic energy for normalization (MeV)
electron_norm_flux = 0 #flux of electrons at normalization energy (cm^-2 sr^-1 s^-1 MeV^-1), 0 turns off normalization
# Switches for elements
#Protons should not be switched off if proton_norm_flux is > 0
max_Z = 0 the largest atomic number (Z) in the nuclear reaction network
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
# Primary abundances
#The abundance ratios are evaluated at the reference energy specified in proton_norm_Ekin
#If normalization at the end of run is turned off (proton_norm_flux = 0), then the absolute values of the
#abundance matter.
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
# Nuclear network settings
#Controls how iterations over the nuclear network is handled. network_iter_compl and network_iter_sec should not be set unless you want to test the code. network iterations should be larger than 20 for damping
#1 iteration should be sufficent for everything else because we now sort the network in order of dependencies.
network_iterations = 1 #number of iterations of protons. Uses larger of network_iterations and network_iter_compl
#network_iter_compl = 1 #number of iterations of complete network, excluding secondary electrons, antiprotons, defaults to min of network_iterations and 2
#network_iter_sec = 1 #number of iterations calculating the secondary productions, defaults to 1. Since the secondaries (excluding nuclei secondaries) don't generate secondaries themselves they should only be calculated once.
total_cross_section = 2 #total cross section option: 0=L83 1=WA96 2=BP01
cross_section_option = 022 #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
warm_start = 0 read in nuclei file and continue run
verbose = 0 -456 -455 -454 -453 verbosity: 0=min,10=max <0: selected debugs
#only used in mapcube or old format
long_min = 0 gamma-ray intensity skymap longitude minimum (deg); 0 -automatic binning required to get correct results!
long_max = 360 gamma-ray intensity skymap longitude maximum (deg); 360 -automatic binning
lat_min = -90 gamma-ray intensity skymap latitude minimum (deg); -90 -automatic binning
lat_max = +90 gamma-ray intensity skymap latitude maximum (deg); +90 -automatic binning
d_long = 4.0 gamma-ray intensity skymap longitude binsize (deg)
d_lat = 4.0 gamma-ray intensity skymap latitude binsize (deg)
