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the initial phase of the project, the theory–experiment feedback loop will be developed using an existing experimental platform whose operation and associated data-analysis methods are already well established
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experimental methods are available and currently fully operational in the laboratory. Collaborative Environment: Centrifugal instabilities are not limited to magnetized plasma columns in the laboratory but also
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experimental research. A high degree of independence will be required to design experiments, identify the most relevant parameters, improve existing setups, and propose new experimental configurations
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model of magmatic oceans on forming planets based on laboratory experiments. At present, high-pressure molten silicates are modelled only in a rudimentary manner, due to a lack of data on activity
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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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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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comparative approach in three South American countries: Brazil, Chile and Colombia. The design of the project is based on a methodology combining three types of research: classic academic, experimental and with
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available. The wet part of the project will be done at the IBPS, and preliminary data demonstrated the feasibility of the project. Indeed, our team has extensive experience in X. laevis embryo dissection
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, etc. from observations collected by one or more instruments, or from numerical experiments. The HP community relies on data centers (such as the CDPP, Centre de Données de la Physique des Plasmas