Detection and characterization of 613 repeating radio burst pairs in the solar corona at 30-50 MHz, with delayed components interpreted as turbulent echoes of harmonic emission via imaging spectroscopy and propagation simulations.
Title resolution pending
2 Pith papers cite this work, alongside 42 external citations. Polarity classification is still indexing.
2
Pith papers citing it
42
external citations · OpenAlex
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.
citing papers explorer
-
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
Detection and characterization of 613 repeating radio burst pairs in the solar corona at 30-50 MHz, with delayed components interpreted as turbulent echoes of harmonic emission via imaging spectroscopy and propagation simulations.
-
Solar Radio Burst Fine Structures
Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.