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We have proposed a novel application for cosmic-ray muography, calledMagic-$\mu$, which is short for Magnetic field Imaging by Cosmic-ray Muons. Thegeneral goal of Magic-$\mu$ is to detect the presence of a magnetic field ormagnetic flux density whose three-dimensional distribution is unknown.Depending on the application, Magic-$\mu$ can have three detection modes. Thefirst is "magnetic field imaging," which is detecting the presence of amagnetic field in specific voxels within a region of space. The other twomodes, transmission and deflection, aim not only to detect the presence butalso to measure the flux density of the magnetic field. We have performed afeasibility study using the PHITS Monte Carlo simulation code, for strong andweak magnetic fields. In this paper, we first give an overview of the conceptand basic principles of magnetic field muography. Then, the results of thefeasibility study on magnetic field imaging for a strong magnetic field (morethan 500 mT) are presented.

Magnetic field imaging by cosmic-ray muons (Magic-$\mu$) -- First feasibility simulation for strong magnetic fields