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DRAGONCELLO code solves the two-dimensional CR transport equation including a fully-anisotropic diffusion tensor (i.e., keeping the assumption of azimuthal symmetry but with orientation of the local magnetic field). This code is presented in: Cerri et al., JCAP 10:019 (2017). Refer to this paper if using DRAGONCELLO.

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sscerr/DRAGONCELLO

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Here a light version of the DRAGON code to propagate a single species with fully anisotropic diffusion

DRAGONCELLO code is presented in: Cerri et al., JCAP 10:019 (2017). Refer to this paper if using this code.

See DRAGONCELLOdocumentation.pdf for installation and compilation guidelines.

Galaxy

  • Fully anisotropic diffusion tensor (depends on local magnetic-field direction)
  • Axisymmetric version of a realistic Galactic magnetic-field model
  • Sources with z and R profile
  • Constant energy losses

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DRAGONCELLO code solves the two-dimensional CR transport equation including a fully-anisotropic diffusion tensor (i.e., keeping the assumption of azimuthal symmetry but with orientation of the local magnetic field). This code is presented in: Cerri et al., JCAP 10:019 (2017). Refer to this paper if using DRAGONCELLO.

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