This is a past event. Its details are archived for historical purposes.
The contact information may no longer be valid.
Please visit our current events listings to look for similar events by title, location, or venue.
Thursday, November 14, 2019 at 4:00pm to 5:00pm
Abstract: The Milky Way is magnetized. Magnetic fields thread the Galaxy, influencing interstellar physics from cosmic ray propagation to star formation. The magnetic interstellar medium (ISM) is also a formidable foreground for observational cosmology, particularly for the quest to find signatures of inflation in the polarized cosmic microwave background (CMB). Despite its importance across scientific realms, the structure of the Galactic magnetic field is not well understood. Observational tracers like polarized dust emission yield only sky-projected, distance-integrated measurements of the three-dimensional magnetic structure. I will discuss new ways to probe the magnetic ISM in three dimensions, by combining high-resolution observations of Galactic neutral hydrogen (HI) with recent insights into how HI morphology encodes properties of the ambient magnetic field. This allows the construction of 3D HI-based Stokes parameter maps: a new tool for studying the structure of the Galactic magnetic field, the ISM, and the polarized foreground to the CMB.