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instruments, such as detectors and lasers operating in the UV to FIR wavelength ranges, fibre-optic sensors, lidars, optical communication systems and quantum technologies. The Section is staffed with around 25
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of the Next Generation Gravity Mission (NGGM) will rely on the high-accuracy measurement of the variation in inter-satellite distance due to the time-varying gravity field via a laser tracking instrument and
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variations using laser interferometry and drag-free control systems. Within NGGM, the Lead Space Segment Engineer supports tasks related to design, development and verification of NGGM satellites within
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. The Section's activities cover the development of novel optical ground stations and related optical systems for optical space debris/near-Earth object observation, satellite and space debris laser ranging and
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Procurement Lead. LISA (Laser Interferometer Space Antenna) is a mission comprising a constellation of three spacecraft tasked with detecting and measuring gravitational waves with precision. It will become
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well as active laser payloads for Earth surface and atmosphere sensing, covering the full wavelength range from ultraviolet to far infrared. You will be involved in the study and pre-development of one or several
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instrumentation. This is particularly relevant for molecular and atomic spectroscopy techniques such as Visible and Near-Infrared (VNIR), Raman, Laser-Induced Breakdown Spectroscopy (LIBS), and X-ray Fluorescence