Exploring the Dynamics of CME-Driven Shocks by Comparing Numerical Modeling and Observations
Abstract
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 multi-messenger observations to explore the role of CME-driven shocks in gamma-ray emissions and SEPs. Motivated by Fermi-LAT long-duration solar flares, we used the AWSoM MHD model to investigate the connection between the shocks and the properties of observed gamma-ray emissions. By coupling the AWSoM with iPATH model, we evaluate the impact of shock evolution complexity near the Sun on SEP intensity and spectra. Our result points to the importance of accurate background coronal and solar wind modeling, as well as detailed observations of CME source regions, in advancing our understanding of CME-driven shocks and the dynamics of associated energetic particles.
Cite
@article{arxiv.2409.18020,
title = {Exploring the Dynamics of CME-Driven Shocks by Comparing Numerical Modeling and Observations},
author = {Meng Jin and Gang Li and Nariaki Nitta and Wei Liu and Vahe Petrosian and Ward Manchester and Christina Cohen and Frederic Effenberger and Zheyi Ding and Melissa Pesce-Rollins and Nicola Omodei and Nat Gopalswamy},
journal= {arXiv preprint arXiv:2409.18020},
year = {2024}
}
Comments
11 pages, 6 figures, to appear in the Proceedings of IAU Symposium No. 388 - Solar and Stellar Coronal Mass Ejections