Kavli Affiliate: Vahe Petrosian | Summary:Shocks driven by coronal mass ejections (CMEs) are primary drivers of gradual solar energetic particle (SEP) events, posing significant risks to space technology and astronauts. Concurrently, particles accelerated at these shocks may also propagate back to the Sun, potentially generating gamma-ray emissions through pion decay. We incorporated advanced modeling and […]
Continue.. Exploring the Dynamics of CME-Driven Shocks by Comparing Numerical Modeling and Observations