The Primordial Magetic Field In The Local Universe
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This dataset contains the 3D structure of large scale magnetic fields in the local Universe, which were seeded by density perturbations during the radiation dominated epoch and later on were evolved by structure formation. This relies on three dimensional initial density fields inferred from the 2M++ galaxy compilation via the Bayesian algorithm. Using those, we estimate the magnetogenesis by the so called Harrison mechanism.<br> <br>
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Zenodo创建时间：
2018-03-07
