
Dates: February 15–19, 2027
Location: University of Tasmania, Hobart, Australia
Optional pre-registration is now closed, but here is the link for posterity. Full registration and abstract submission will follow later in 2026, open to anyone regardless of whether you pre-registered.
Contact the organizing committee at hobart-magnetism-soc at lists.ubc.ca.
Topics
The scientific organising committee has identified a number of scientific and technical questions to give a flavour for the topics we hope to investigate at the meeting
- Scientific questions
- Structure of magnetic fields in the Milky Way
- Large-scale structure
- Structure in the solar neighbourhood
- Connection of magnetic fields to discrete ISM structures
- Properties of the Local Bubble
- How large-scale magnetic field connects to smaller cloud/envelope scales
- How large-scale magnetic field connects to smaller cloud/envelope scales
- Energy balance / partition in diffuse ISM
- Relative orientation of 3D field with respect to density structures
- Properties of the Local Bubble and its impact on Galactic and extragalactic observations
- Dynamical impact of magnetic fields on star formation and galaxy evolution
- Impact of the Local Bubble on Galactic and extragalactic observations
- Dynamical impact of magnetic fields on star formation and galaxy evolution
- Structure of magnetic fields in the Milky Way
- Technical questions
- Large-scale diffuse emission: single antennas and interferometers
- Combining surveys across wavelengths (eg GMIMS low-GMIMS high; LOFAR-GMIMS low)
- Combining surveys across latitudes (eg GMIMS high band north-GMIMS high band south)
- QU fitting vs Faraday synthesis
- How do we separate foreground emission for extragalactic/distant Galactic studies?
- What information can we extract by comparing RM-grids with diffuse emission?
- Preparation for large-scale data expected from next-generation telescopes (especially SKA)
- m-mode imaging
- Large-scale diffuse emission: single antennas and interferometers
Format
The workshop will consist of a relatively limited number of talks, likely roughly three hours per day. After formal talks, there will be significant time for collaboration and topical discussions.
Scientific Organising Committee
Alex S Hill (UBCO, co-chair)
Jennifer West (U Tasmania, co-chair)
Craig Anderson (ANU)
Vibor Jelic (Ruđer Bošković Institute)
Amit Seta (ANU)
Mehrnoosh Tahani (U South Carolina)