SEAMS SCHOOL FINAL REPORT

In this school, we introduced the basis of the mathematical analysis to study differential equations (ordinary and partial). One aim to prepare students and staff members for more concrete problems arising in mathematical modeling in engineering and biological processes. Theoretical and numerical lectures were given, with a presentation of free scientific computing software using Python. A website and a drive were created to facilitate exchanges between students, lecturers and organizers: The school was sponsored by CIMPA (Centre International de Mathématiques Pures et Appliquées) IMU (International Mathematical Union) ISP (International Science Programme) NUOL (National University of Laos) Erasmus Mundus ERDF – Picardie Region Beerlao ETL3G

ISM simulations: an overview of models

Until recently the dynamical evolution of the interstellar medium (ISM) was simu- lated using collisional ionization equilibrium (CIE) conditions. However, the ISM is a dynamical system, in which the plasma is naturally driven out of equilibrium due to atomic and dynamic processes operating on different timescales. A step forward in the field comprises a multi-fluid approach taking into account the joint thermal and dynamical evolutions of the ISM gas.