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| author | Aaron LI <aly@aaronly.me> | 2017-07-26 15:58:51 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2017-07-26 15:58:51 +0800 |
| commit | 2e089e03fdeb0fc5bde86cd5fd93e16a42983a79 (patch) | |
| tree | 8691b7ee79705e7151862670d0e0df09ab9be168 /fg21sim | |
| parent | e6b727785fab339103a103194317ffdc6ba37684 (diff) | |
| download | fg21sim-2e089e03fdeb0fc5bde86cd5fd93e16a42983a79.tar.bz2 | |
clusters/halo.py: Add property "magnetic_field"
Signed-off-by: Aaron LI <aly@aaronly.me>
Diffstat (limited to 'fg21sim')
| -rw-r--r-- | fg21sim/extragalactic/clusters/halo.py | 11 |
1 files changed, 11 insertions, 0 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py index 7c52f97..44d1e1a 100644 --- a/fg21sim/extragalactic/clusters/halo.py +++ b/fg21sim/extragalactic/clusters/halo.py @@ -162,6 +162,17 @@ class RadioHalo: r_halo = helper.radius_halo(mass, self.z_merger) # [kpc] return r_halo + @property + def magnetic_field(self): + """ + The magnetic field strength at the simulated observation + time (i.e., cluster mass of ``self.M_obs``), will be used + to calculate the synchrotron emissions. + + Unit: [uG] + """ + return helper.magnetic_field(self.M_obs) + def calc_electron_spectrum(self, zbegin=None, zend=None, n0_e=None): """ Calculate the relativistic electron spectrum by solving the |