Nature Communications, Published online: 09 June 2026; doi:10.1038/s41467-026-74137-2 Solar radio bursts often exhibit complex fine structures that encode crucial coronal dynamics. Here, the authors report the detection of spike-like repeating burst pairs and show that the delayed component arises from anisotropic scattering of harmonic emission, revealing coronal turbulence and high-altitude magnetic reconnection.
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
Yihua Yan
