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| author | Aaron LI <aly@aaronly.me> | 2017-07-21 23:52:24 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2017-07-21 23:52:24 +0800 |
| commit | 0a3555701177f7cb6e802317ba67516d5d865fd5 (patch) | |
| tree | 50bc9bfcf5934aa734dca117ce361191c044acb1 /fg21sim/configs/20-extragalactic.conf.spec | |
| parent | a65642405fe1653325d3560a2d47949c1f05810a (diff) | |
| download | fg21sim-0a3555701177f7cb6e802317ba67516d5d865fd5.tar.bz2 | |
clusters/main.py: Add "_magnetic_field()" method
Also update the configurations
Signed-off-by: Aaron LI <aly@aaronly.me>
Diffstat (limited to 'fg21sim/configs/20-extragalactic.conf.spec')
| -rw-r--r-- | fg21sim/configs/20-extragalactic.conf.spec | 15 |
1 files changed, 7 insertions, 8 deletions
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec index 0f797a8..b8af33b 100644 --- a/fg21sim/configs/20-extragalactic.conf.spec +++ b/fg21sim/configs/20-extragalactic.conf.spec @@ -43,6 +43,13 @@ # The fraction that a cluster hosts a radio halo halo_fraction = float(default=None, min=0.0, max=1.0) + # Magnetic field scaling relation for clusters + # Reference: Cassano et al. 2012, A&A, 548, A100, Eq.(1) + # + # The mean magnetic field assumed + b_mean = float(default=1.9, min=0.1, max=10) + # The index of the scaling relation + b_index = float(default=1.5, min=0.0, max=3.0) # Resolution for simulating each cluster templates, which are finally # mapped to the all-sky HEALPix map if used. @@ -73,14 +80,6 @@ # XXX: currently only support a constant radius of halos radius = float(default=500.0, min=100.0) - # Magnetic field scaling relation for clusters - # Reference: Cassano et al. 2012, A&A, 548, A100, Eq.(1) - # - # The mean magnetic field assumed - b_mean = float(default=1.9, min=0.1, max=10) - # The index of the scaling relation - b_index = float(default=1.5, min=0.0, max=3.0) - # Fraction of the turbulence energy in the form of magneto-sonic waves. eta_t = float(default=0.3, min=0.0, max=1.0) |