Plasma interactions of exoplanets with their parent star and associated radio emissions

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Searching for star–planet interactions within the magnetosphere of HD 189733 (2010, background): “The amount of power emitted by radio waves Prad is roughly proportional to the power input Pinput supplied by the stellar wind magnetic energy (see Figure 6 Zarka 2007).”
Magnetic energy fluxes in sub-Alfvénic planet star and moon planet interactions (2013, background): “These expressions differ from the expressions in Zarka (2007) and Lanza (2009) A119, page 7 of 20 next to other details by a factor of 2v/vA.”
Science with a lunar low-frequency array: From the dark ages of the Universe to nearby exoplanets (2009, background): “Of particular interest for a lunar array are studies of the earliest phase of the universe which are not easily accessibleby other means.”
Dynamo Scaling Laws and Applications to the Planets (2010, background): “Saturn is similar to Jupiter in its internal structure, which comprises a large core region of metallic hydrogen (Fortney and Nettelmann 2009, this issue).”
Predicting low-frequency radio fluxes of known extrasolar planets (2007, methodology): “For this reason, the most appropriate frequency window for radio observations seems to be between 10 and 70 MHz.”