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Lookup NU author(s): Dr Luiz Felippe RodriguesORCiD, Dr Luke Chamandy


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Computes time and radial dependent magnetic fields for a sample of galaxies in the output of a semi-analytic model of galaxy formation. The magnetic field is obtained by numerically solving the galactic dynamo equations throughout history of each galaxy. Stokes parameters and Faraday rotation measure can also be computed along a random line-of-sight for each galaxy.

Publication metadata

Programmer(s): Rodrigues LFS, Chamandy L

Publication type: Software

Publication status: Published

Year: 2019

Online publication date: 15/06/2019


DOI: 10.5281/zenodo.3246748