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A monitoring campaign (2013-2020) of ESA's Mars Express to study interplanetary plasma scintillation

Bocanegra-Bahamón, T. M.; Molera Calvés, G.; Duev, D. A. +19 more

The radio signal transmitted by the Mars Express (MEX) spacecraft was observed regularly between the years 2013-2020 at X-band (8.42 GHz) using the European Very Long Baseline Interferometry (EVN) network and University of Tasmania's telescopes. We present a method to describe the solar wind parameters by quantifying the effects of plasma on our r…