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Magnetic fields play essential roles in various astronomical objects. Radioastronomy has revealed that magnetic fields are ubiquitous in our Universe.However, the real origin and evolution of magnetic fields is poorly proven. Inorder to advance our knowledge of cosmic magnetism in coming decades, theSquare Kilometre Array (SKA) should have supreme sensitivity than ever before,which provides numerous observation points in the cosmic space. Furthermore,the SKA should be designed to facilitate wideband polarimetry so as to allow usto examine sightline structures of magnetic fields by means of depolarizationand Faraday Tomography. The SKA will be able to drive cosmic magnetism of theinterstellar medium, the Milky Way, galaxies, AGN, galaxy clusters, andpotentially the cosmic web which may preserve information of the primevalUniverse. The Japan SKA Consortium (SKA-JP) Magnetism Science Working Group(SWG) proposes the project "Resolving 4-D Nature of Magnetism withDepolarization and Faraday Tomography", which contains ten scientific usecases.

Resolving 4-D Nature of Magnetism with Depolarization and Faraday Tomography: Japanese SKA Cosmic Magnetism Science