Magnetic field and ISM in the local Galactic disc
  Correlation analysis is obtained among Faraday rotation measure, HI column
density, thermal and synchrotron radio brightness using archival all-sky maps
of the Galaxy. A method is presented to calculate the magnetic strength and its
line-of-sight (LOS) component, volume gas densities, effective LOS depth,
effective scale height of the disk) from these data in a hybrid way. Applying
the method to archival data, all-sky maps of the local magnetic field strength
and its parallel component are obtained, which reveal details of local field
orientation.
