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Interstellar magnetic fields play critical roles in many astrophysicalprocesses. Yet despite their importance, our knowledge about magnetic fields inour Galaxy remains limited. For the field within the Milky Way, much of what wedo know comes from observations of polarisation and Faraday rotation measures(RMs) of extragalactic sources and pulsars. A high angular density of RMmeasurements in several critical areas of the Galaxy is needed to clarify theGalactic magnetic field structure. Using observations made with the VLA, wehave determined RMs for sources in regions of the Galactic plane not covered bythe Canadian Galactic Plane Survey (CGPS) and Southern Galactic Plane Survey(SGPS). We have combined these new RMs with those determined from the CGPS andSGPS and have produced a new model for the magnetic field of the Galactic disk.

Modeling the Galactic Magnetic Field using Rotation Measure Observations in the Galactic Disk from the CGPS, SGPS, and the VLA