Description
The goal of the program is to achieve tangible progress in our understanding of the structure and origin of the Milky Way’s magnetic field, to pave the way for further progress in this direction, and to address a range of fundamental questions in other areas of galactic astrophysics that have magnetic fields and cosmic rays at their core. Specific questions include: What are the properties of magnetohydrodynamic turbulence in the interstellar medium? What can we learn from the observations of other galaxies (and contribute to) galaxy formation theory? What is the interplay between cosmic structure, magnetic fields and the origin and propagation of extragalactic cosmic rays? Answers to these question, even if partial and incomplete, would advance fundamentally our understanding of galactic magnetic fields, bring closer their theory, simulations and observations, and inform crucially the rapidly evolving concepts in galaxy formation and evolution.| Period | 3 Apr 2023 → 28 Apr 2023 |
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| Event type | Conference |
| Location | Stockholm, SwedenShow on map |
| Degree of Recognition | International |