A model of specular stellar radio reflection from the ionosphere of the hot Jupiter HD189733b predicts a reflected flux of 0.01 to 0.05 percent of the stellar flux at 50 MHz, detectable only for exceptionally bright radio stars with very long integrations.
K., Trivedi , R., & Vats , H
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Observability of radio reflections from exoplanet ionospheres with next generation radio telescopes
A model of specular stellar radio reflection from the ionosphere of the hot Jupiter HD189733b predicts a reflected flux of 0.01 to 0.05 percent of the stellar flux at 50 MHz, detectable only for exceptionally bright radio stars with very long integrations.