CORDIS Project
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This project investigates the Galactic magnetic field using advanced modeling and large datasets from polarized stars. By employing Bayesian statistics, it aims to create a comprehensive 3D model of dust distribution and magnetic turbulence in the Galaxy, enhancing our understanding of cosmic phenomena.
What makes our Galaxy’s ecosystem so fascinating is the complex interactions between its components: stars, gas, dust, magnetic fields, and cosmic rays.
Of these components, the Galactic magnetic field (GMF) may well be the most enigmatic.
Only partially observable through indirect means, its study relies heavily on modeling, almost exclusively using line-of-sight integrated radio-polarimetric data.
Although much has been learned, many questions are still unanswered especially about the turbule…
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