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staff members (researchers, engineers, PhD students) and operates several major experimental facilities: LULI2000, Apollon, HERA, XCAN. The PhD student will join LULI's theory team (TIPS) and will work
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an exceptional know-how and experimental methodology, in a high-level scientific environment. The context of frequency metrology requires to master and control the noise sources of the experimental setup as
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for analyzing the experimental data obtained. In a second phase, the experience gained from the implementation of this first test cryostat will enable the PhD student to contribute to defining
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staff of around 120, including 66 permanent staff. It has a strong experimental component, with numerous prototype set-ups supported by both standard equipment and high-tech instrumentation
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Circulation Model (GCM) outputs, followed by forcing a glaciological model through parameter perturbation experiments. The student will benefit from outputs of the IPSL model and sensitivity tests developed as
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training that includes courses in planetology and planetary plasmas. • The student can demonstrate research experience (M1 and/or M2 internships) on a topic related to planetology and/or space plasmas
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of Research Experience1 - 4 Research FieldSociologyYears of Research Experience1 - 4 Additional Information Eligibility criteria Education: Ph.D. in ecology, geography, or environmental sciences with experience
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collaboration with Osaka University, where in situ kinetic measurement experiments can be conducted. Finally, this thesis is part of the ANR MUSiCAL project, a collaborative initiative between SIMaP (Université
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combine laboratory experiments, numerical simulations, artificial intelligence and field observations to address outstanding questions in physical oceanography, atmospheric sciences, physical limnology
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project, which aims to use interglacial and millennial-scale climate changes of the last 220,000 years as natural experiments to provide the first integrated understanding of atmosphere-land-ocean