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are often accompanied by turbulent sheath regions—zones of compressed plasma and magnetic fields formed between the CME-driven shock and the CME itself. While sheath regions are known to play a major role in
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reconstitution, cell biology, and fluorescence microscopy imaging tools, we aim to uncover how protein-membrane interactions promote membrane microdomain formation and how these structures respond to external
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conditions (around 0.1 au from the Sun). By combining high-resolution remote sensing data (especially EUV spectral imaging) with advanced simulations, RIB-Wind seeks to more accurately characterize the solar
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