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their detection, (iv) enabling better analysis of exoplanetary radio emissions. • Use of data from the Juno/Waves mission and solar wind propagation models • Understanding the visibility biases of the various
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stimulated Raman scattering and two-plasmon decay, which involve Langmuir waves, as well as stimulated Brillouin scatter-ing and cross-beam energy transfer (CBET), which involve the ion acoustic response
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at the Laplace laboratory, where numerical and analytical models are being developed to predict plasma potential control and flux entrainment from polarized electrodes. During the third year of the thesis project
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