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Fig. 3

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Examples of dynamic spectra of Jupiter recorded by the NDA with its Routine receiver. The top panel illustrates the ionospheric and RFI conditions at night. The bottom panel illustrates those conditions during daytime. Vertical lines are calibration sequences. Jupiter’s decameter emission is structured in “arcs” in the t-f plane. The horizontal black lines are RFI. This figure is adapted from Lecacheux (2000).

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