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stars experience a radically different environment than those around main-sequence stars, as intense stellar winds, high mass-loss rates, and extended atmospheres can strongly affect planetary atmospheres
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or damage. Along these lines, this project develops SHM methods for deep tunnels, with the HADES Underground Research Laboratory (URL) serving as the primary case study. The monitoring strategy combines in
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the ERC project, such as qualitative data collection, analysis, and integration of findings. You will support the Principal Investigator (PI) and actively participate in the collaborative and
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