I am trying to model gamma ray emission around Pulsar. Similar model as in paper "Johannesson, Porter & Moskalenko, The ApJ, 879:91 (2019)" about Geminga.
The question is where in the code/galdeffile can I find option to change the parameter D_z - diffusion coefficient in SDZ (slow diffusion region)? This parameter occurs in the formula 3 from aforementioned paper, here is the image with this formula where one can find this parameter D_z:
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Screenshot 2022-06-27 at 15.48.28.png [ 28.2 KiB | Viewed 11963 times ]