SIMBAD references

We discuss observations of the linearly polarized component of the diffuse galactic radio background. These observations, with an angular resolution of 4', were made with the Westerbork Synthesis Radio Telescope (WSRT) in 5 frequency bands in the range 341-375MHz. The linearly polarized intensity P (with polarized brightness temperature going up to 10K) shows a `cloudy' structure, with characteristic scales of 15-30', which contains relatively long, but very narrow `canals' (essentially unresolved) in which P is only a small fraction of that in the neighbouring beams. These `canals' are generally seen in more than one frequency band, although their appearance changes between bands. They are probably due to depolarization within the synthesized beam, because the change in polarization angle Δφ<sub>pol</sub> across the deepest `canals' is in general close to 90° (or 270° etc.). These very abrupt changes in φ_pol, which are seen only across the `canals', seem to be accompanied by abrupt changes in the Rotation Measure (RM), which may have the right magnitude to create the difference of close to 90° in φ<sub>pol</sub>, and thereby the `canals'. The structure in the polarization maps is most likely due to Faraday rotation modulation of the probably smooth polarized radiation emitted in the halo of our Galaxy by the fairly local (≲500pc) ISM. Therefore, the abrupt changes of RM across the `canals' provide evidence for very thin (≲1pc), and relatively long transition regions in the ISM, across which the RM changes by as much as 100%. Such drastic RM changes may well be due primarily to abrupt changes in the magnetic field.