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authorAaron LI <aly@aaronly.me>2019-02-27 11:05:50 +0800
committerAaron LI <aly@aaronly.me>2019-02-27 14:05:49 +0800
commit5498d4224f5c386675ba0b0e017c1cabff51a7a2 (patch)
tree897f75871f222c022ff5fe9366e84ac8214f4874 /fg21sim
parent2dfd5c5b410a8c6f4c4a5f79671374e4a14d60f0 (diff)
downloadfg21sim-5498d4224f5c386675ba0b0e017c1cabff51a7a2.tar.bz2
configs/spec: Reorder options to be clearer
Diffstat (limited to 'fg21sim')
-rw-r--r--fg21sim/configs/config.spec30
1 files changed, 14 insertions, 16 deletions
diff --git a/fg21sim/configs/config.spec b/fg21sim/configs/config.spec
index 081565f..74abb69 100644
--- a/fg21sim/configs/config.spec
+++ b/fg21sim/configs/config.spec
@@ -387,26 +387,24 @@ stream = option("stderr", "stdout", "", default="stderr")
# Giant radio halos
#
[[halos]]
- # A custom factor to tune the turbulent acceleration efficiency.
- # NOTE: This parameter incorporates the efficiency factor describing
- # the effectiveness of the ICM plasma instabilities.
- f_acc = float(default=0.1, min=0.1, max=10)
+ # The fraction of the thermal energy injected into the cosmic-ray
+ # electrons during the cluster life time.
+ eta_e = float(default=0.001, min=0, max=1)
+ # The spectral index of the injected primary electrons.
+ injection_index = float(default=2.3, min=2, max=3)
- # The factor that is multiplied to the turbulence injection radius
- # to derive the radio halo radius.
- f_radius = float(default=0.7, min=0.1, max=10)
+ # The fraction of merger energy transferred into the turbulence.
+ eta_turb = float(default=0.15, min=0, max=1)
# The base energy fraction of the turbulence to the ICM thermal energy
# (for a relaxed system).
# x_turb ~< 5% [Vazza et al. 2011, A&A, 529, A17]
x_turb = float(default=0.01, min=0, max=0.5)
- # The fraction of merger energy transferred into the turbulence.
- eta_turb = float(default=0.15, min=0, max=1)
-
- # The fraction of the thermal energy injected into the cosmic-ray
- # electrons during the cluster life time.
- eta_e = float(default=0.001, min=0, max=1)
+ # A custom factor to tune the turbulent acceleration efficiency.
+ # NOTE: This parameter incorporates the efficiency factor describing
+ # the effectiveness of the ICM plasma instabilities.
+ f_acc = float(default=0.1, min=0.1, max=10)
# The energy density ratio of cosmic ray to the thermal ICM.
# NOTE: Equipartition between the magnetic field and cosmic ray is
@@ -417,13 +415,13 @@ stream = option("stderr", "stdout", "", default="stderr")
# mass of the cluster.
mass_index = float(default=0, min=0, max=3)
+ # The factor that is multiplied to the turbulence injection radius
+ # to derive the radio halo radius.
+ f_radius = float(default=0.7, min=0.1, max=10)
# The scaling index of the halo radius (R_halo) w.r.t. the virial
# radius of the cluster.
radius_index = float(default=1.7, min=0, max=3)
- # The spectral index of the injected primary electrons.
- injection_index = float(default=2.3, min=2, max=3)
-
# Minimum and maximum Lorentz factor (i.e., energy) of the relativistic
# electron spectrum.
gamma_min = float(default=1)