EGAS41 - Swansea University
EGAS41 - Swansea University
EGAS41 - Swansea University
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41 st EGAS CP 7 Gdańsk 2009<br />
Ne I excitation rate coefficients for C-R models applied to<br />
electric propulsion<br />
Ch. Berenguer 1 , K. Katsonis 1 , R.E.H. Clark 2<br />
1 GAPHYOR, Laboratoire de Physique des Gaz et des Plasmas, UMR 8578, Université<br />
Paris-sud, 91405 Orsay cedex, France<br />
2 Nuclear Data Section, IAEA, Wagramerstr. 5, A-1400 Vienna, Austria<br />
∗ Corresponding author: konstantinos.katsonis@u-psud.fr,<br />
Because of the possible use of Ne as a fuel gas in electric propulsion devices, we are<br />
developing a Collisional-Radiative (C-R) model valid for low temperature Ne plasma,<br />
encompassing the neutral Ne atom and its first ion, with Ne III as a continuum [1].<br />
This “zero dimension” model is meant for non-intrusive emission spectroscopy diagnostics<br />
giving the local electronic temperature T e and density n e inside a plasma thruster; it<br />
can also be used as a basis for development of a detailed full dimensional model [2].<br />
Validation of the C-R model is underway, mainly by use of a Ne-filled hollow cathode lamp<br />
experimental facility in which the positions and intensities of the principal Ne I and Ne II<br />
spectral lines have been measured. The theoretical spectra obtained by the C-R model rely<br />
on transition probability (A ij ) and electron impact collision excitation (σ e ) data. In the<br />
present contribution we focus on evaluation of the σ e and of the corresponding excitation<br />
rates for the lower levels of Ne I. In addition to the available experimental and theoretical<br />
results [3], we have used the following theoretical methods [4] for the σ e evaluations: i)<br />
The Born approximation (high energy region) in which the structure parameters are of<br />
paramount importance. ii) Distorted Wave (DW) approximation and First Order Many<br />
Body Theory (FOMBT) at electron impact energies approaching the threshold, using<br />
the online interface to the Los Alamos National Laboratory atomic physics codes [5].<br />
iii) Quasi-classical evaluations based on the Hamiltonian formulation of the few body<br />
problem, following numerical CTMC studies.<br />
Acknowledgment<br />
The research leading to these results has received funding from the European Community’s<br />
Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 218862.<br />
References<br />
[1] Ch. Berenguer, K. Katsonis, S. Cohen, P. Tsekeris, M. Cornille, A Collisionnal-<br />
Radiative Model for Low Temperature Ne Plasmas, 31 st IEPC, Ann Arbor, MI USA<br />
[2] K. Katsonis, S. Pellerin, K. Dzierzega, JHTMP 7, 559 (2003)<br />
[3] M.H. Phillips, L.W. Anderson, Chun C. Lin, Phys. Rev. A 12 (1985); M. Allan et al.,<br />
J. Phys. B 42 044009 (2009) and references therein<br />
[4] Ch. Berenguer, Optical Diagnostics of High Energy Density Plasmas, PhD Thesis,<br />
Orsay, February 2009<br />
[5] http://aphysics2.lanl.gov/tempweb/<br />
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