Neutron stars, despite being composed primarily of neutrons, can produce magnetic fields due to the presence of quarks within the neutrons that carry electric charge. The crust of a neutron star is believed to contain a layer of iron and possibly superfluid protons, which could contribute to its magnetic field through electric currents. The internal structure of neutron stars includes a mix of protons and neutrons, allowing for conductivity and potential superconductivity under extreme pressures. The magnetic moment of neutrons may also play a role in trapping magnetic fields, independent of the crust's involvement. The complexities of neutron star physics, including the poorly defined equation of state, leave many aspects speculative.