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Wave and turbulent phenomena occur ubiquitously in all types of solar-terrestrial plasmas, ranging from the Sun, solar wind, magnetosphere to the ionosphere. The meeting aims to compare theoretical and observational results from the different disciplines, share analysis techniques and address interdisciplinary questions such as properties of waves in energetic processes, the solar origin of turbulence in the solar wind and the solar wind drivers of magnetospheric pulsations and ionospheric turbulence.
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