How local is the local interstellar magnetic field
Similar directions are obtained for the local interstellar magnetic field (ISMF) by comparing diverse data and models that sample five orders of magnetic in spatial scales. These data include the ribbon of energetic neutral atoms discovered by the Interstellar Boundary Explorer, heliosphere models, the linear polarization of light from nearby stars, the Loop I ISMF, and pulsars that are within 100–300 pc. Together these data suggest that the local ISMF direction is correlated over scales of ~ 100 pc, such as would be expected for the interarm region of the galaxy.