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.
Astronomy & astrophysics43(2), 201–214 (1975)
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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.