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author | Aaron LI <aly@aaronly.me> | 2017-10-20 10:22:24 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-10-20 10:22:24 +0800 |
commit | fd20ab688759f3dfc3f7796ac0b1118e21ee5b22 (patch) | |
tree | a75ffd2b7ae280afe65b71e998b0da22c7e7fde1 /fg21sim/uvsim | |
parent | 283ca6c00e5ff6c74b529d0a460115516c16eec7 (diff) | |
download | fg21sim-fd20ab688759f3dfc3f7796ac0b1118e21ee5b22.tar.bz2 |
clusters/halo: Determine magnetic field by fraction of its energy density
* Rewrite "magnetic_field()" function to calculate the mean magnetic field
strength within ICM according its energy density fraction w.r.t. the ICM
thermal energy density.
* Remove config options "b_mean" and "b_index", which are replaced with the
option "eta_b", the assumed magnetic energy density fraction w.r.t. the
ICM thermal energy density.
Diffstat (limited to 'fg21sim/uvsim')
0 files changed, 0 insertions, 0 deletions