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Content archived on 2022-12-23

Earth space plasma via computer simulation

Objective



The purpose of this network programme is to promote the use of computer simulation in order to improve our understanding of intricate non-linear physical processes that commonly appear in space plasmas. Numerical simulation has become a very powerful tool for analysing a large number of various phenomena that take place in many subfields of plasma physics. With the help of recent computers, such a tool presents the enormous advantage of being able to reproduce various natural plasma phenomena, as well as active space experiments on board satellite missions. In other words, it represents a diagnostic tool that is powerful and quite complementary to theoretical and experimental analysis. One of the main advantages is to follow (weak or strong) non-linear stages of plasma physics which are very difficult to analyse simply by theoretical approaches.

This project will focus on outstanding and selected phenomena, based on the fact that these can be applied in different areas of space plasma physics. These topics and expected results are: simulations of beam-plasma interaction: establishment of a single solitary structure in 3-D (simulations with KARAT code); a better understanding of the use of statistical properties of the structure for the beam relaxation theory; tearing instabilities in the magnetospheric tail: the establishment of the equilibrium system in the simulations; a better understanding of the test particle acceleration in the reconnection configuration. In studying the evolution of plasma clouds the 2-D version can be used for planar and cylinder expansions and the 3-D version can be used for spherical expansion; further research will be on the inclusion of appropriate boundary conditions in 2-D and 3-D versions of the KARAT code Preliminary results on dimensionality effects with a 2-D and 3-D release by comparison with 1-D release are already known and developed on Active Magnetospheric Particle Tracer Explorer mission (AMPTE) and Combined Release and Radiation Effects Satellite mission (CRESS) space experiments.

In addition, the project will also encourage the exchange of mathematical/numerical techniques used in specific numerical codes. Some effort will be also devoted to new and/or recent diagnosis methods in the post-processing stage of numerical results.

A workshop meeting will be held in Paris in order to evaluate the results of this research project.

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Programme(s)

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Topic(s)

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Call for proposal

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Funding Scheme

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Coordinator

Centre National d'Etudes des Télécommunications
EU contribution
No data
Address
Rue du Général Leclerc 38-40
92131 Issy-les-Moulineaux
France

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Total cost

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Participants (3)

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