Et-Touhami ES-SEBBAR

En résumé

Entreprises

• Paul Scherrer Institute - Scientist

  2015 - maintenant

• Laboratory of Gas and Plasma - Research Scientist

  2014 - 2015 "Study of micro-plasma jets, chemistry and their fundamental phenomena using laser spectroscopy and fast imaging" Laboratory of Gas and Plasma Physics (LPGP), CNRS - UMR 8578, University of Paris 11, 91405, Orsay, France

• University of Paris Est- Créteil (UPEC) - Teaching Assistant

  2014 - 2015 Teaching assistant for the course of Physics, Engineering, Mechanics and Electronic (students in L1 & L2 levels).

• King Abdullah University of Science and Technology - Postdoctoral Fellow

  2010 - 2014 Chemical Kinetics & Laser Sensors

• LATMOS laboratory - Postdoctoral Fellow

  2010 - 2010 Titan's atmosphere

• the University of Paris Est- Créteil - Teaching Assistant

  2009 - 2010 Teaching assistant for the course of Physics, Engineering, Mechanics, Electronic and Informatics (students in L2 & L3 levels).

• Créteil - Teaching Assistant

  2008 - 2009 Physics and chemistry

• Laboratoire Inter-universitaire des systèmes atmosphériques - Postdoctoral Fellow

  2007 - 2009 Chemistry in Titan's atmosphere

• CNRS - Postdoctoral Fellow

  Paris 2007 - 2009 The SETUP program consists of a reactor where the initial gas mixture (nitrogen N2 and methane CH4, the constituents of the atmosphere of the Titan satellite) are exposed, for the first time, to both of the major energy sources (i.e. electrons and photons) responsible for the chemical evolution of Titan's atmosphere. A flowing microwave cold plasma and its afterglow are settled in order to dissociate N2 and production of N atoms, while UV photons delivered by a continuous lamp (@Lyman =121.6 nm) or a pulsed Excimer laser (@ 248 nm) are used to dissociate CH4 (by a 1 and a 2 photons mechanism, respectively). The chemistry of nitrogen and photochemistry of methane are combined. The resulting complex chemistry between N atoms and CH3, CH2, CH fragments are probed thanks to in-situ time resolved laser spectroscopy (CRDS) in infrared spectral range. Time resolved analysis of intermediates species as well as primary products are carried out in order to identify the chemical mechanisms taking place in Titan satellite. In parallel to the SETUP project, I participated at various measurement campaigns using Synchrotron radiations (Bessy-Berlin, Germany and at Soleil - Paris, France) as a tunable VUV light source for absorption cross-sections of nitriles and hydrocarbons in VUV range at different temperatures.

Formations

• University Of Paul Sabatier

  Toulouse 2003 - 2007 Doctor of Philosophy
  
  "Physics of Plasmas and Engineering"
  Laboratory of Plasma and Conversion of Energy (LAPLACE), University of Paul Sabatier

• University Of Paul Sabatier

  Toulouse 2002 - 2003 Masters Degree
  
  Master's degree in "Physics of Plasmas and Engineering" Laboratory of Plasma and Conversion of Energy (LAPLACE), University of Paul Sabatier.

Réseau

• Amal EL MZABI

• Emilie BRIÉ