Eleonora Puzzoni

I am currently a Postdoctoral Research Associate at the Laboratorie Lagrange (Observatoire de la Côte d’Azur) modeling  cosmic ray transport across our turbulent galaxy as part of the MiCRO project.

After working as a Postdoctoral Research Associate, I currently serve as a Designated Campus Colleague at the Lunar and Planetary Laboratory, University of Arizona, as part of the Solar and Heliospheric Research Group, investigating the transport of GeV-TeV galactic cosmic rays and modeling the gamma-ray emission from the solar disk observed by the Fermi Gamma-ray Space Telescope and the HAWC observatory (previously supported by NASA under grant 80NSSC22K0040). 

I am also a member of the SHIELD NASA Drive Center team, where I am involved in developing a Galactic Cosmic Rays Webtool.

I have always been fascinated and passionate about high-energy astrophysical phenomena such as gamma-ray bursts, blazar, and supernova remnants. In particular, I am interested in studying particle transport and acceleration through magnetohydrodynamic (MHD) numerical simulations, with a keen interest in exploring the role of magnetic reconnection in these processes.