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astro-ph.SR2025
Comprehensive study of solar type II radio bursts and the properties of the associated shock waves
K. Bhandari, D. E. Morosan, S. Normo
Type II radio bursts are solar radio emissions generated by electrons accelerated by coronal shocks. These bursts are typically found close to expanding coronal mass ejections (CME…
astro-ph.SR2025★ 3 cited
Imaging and spectropolarimetric observations of a band-split type II solar radio burst with LOFAR
S. Normo, D. E. Morosan, P. Zhang +2
Type II solar radio bursts are generated by electrons accelerated by coronal shock waves. They appear in dynamic spectra as lanes drifting from higher to lower frequencies at the p…