Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session JP11: Poster Session IV: Education and Outreach; Undergraduate or High School Research; Plasma technology, Fusion reactor Nuclear and Materials Science; Propulsion; Materials Interfaces (2:00pm-5:00pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.JP11.35
Abstract: JP11.00035 : Modeling the transition from a space-charge limited sheath to an inverse sheath**
Presenter:
Grant Johnson
(Lawrence Livermore National Laboratory)
Authors:
Grant Johnson
(Lawrence Livermore National Laboratory)
Michael Campanell
(Lawrence Livermore National Laboratory)
It was recently discovered that charge-exchange collisions in a space-charge limited (SCL) sheath force a transition to the inverse sheath regime [1]. The collisions cause ions to become trapped in the potential well of the SCL sheath. The accumulating ions neutralize part of the charge in the sheath, collapsing the double layer region and leaving behind an inverse sheath. In experiments looking for a specific regime, it is important to consider the time scale of the transition relative to experimental time scales. Depending on the plasma properties, collision rates and emission parameters, the time required for a transition from the SCL to inverse sheath can span many orders of magnitude. We have developed an analytical model of the SCL-to-inverse transition and tested it against 1D-1V simulations. The model calculations involve additional analytic approximations of useful quantities including the total charge in the layers of a SCL sheath, the length of the virtual cathode, and the length of an inverse sheath. [1] M. D. Campanell and M. V. Umansky, Physics of Plasmas 24, 057101 (2017).
**This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.JP11.35
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