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 TP11: Poster Session VII: Basic Plasma Physics: Pure Electron Plasma, Strongly Coupled Plasmas, Self-Organization, Elementary Processes, Dusty Plasmas, Sheaths, Shocks, and Sources; Mini-conference on Nonlinear Waves and Processes in Space Plasmas - Posters; MHD and Stability, Transients (2), Runaway Electrons; NSTX-U; Spherical Tokamaks; Analytical and Computational Techniques; Diagnostics (9:30am-12:30pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.TP11.32
Abstract: TP11.00032 : Formation of Hollow Density Profile in Magnetically Expanding Plasma Produced by Helicon Antenna
Presenter:
Sonu Yadav
(Institute for Plasma Research, HBNI, Gandhinagar)
Authors:
Sonu Yadav
(Institute for Plasma Research, HBNI, Gandhinagar)
Soumen Ghosh
(Department of Physics, University of California, San Diego)
Sayak Bose
(Columbia Astrophysics Laboratory, Columbia University)
Kshitish Kumar Barada
(Department of Physics and Astronomy University of California, Los Angeles)
Prabal Kumar Chattopadhyay
(Institute for Plasma Research, HBNI, Gandhinagar)
The radial density profile in the magnetic nozzle of the Helicon eXperimental (HeX) device is found to be modified from being centrally peaked to that of hollow nature as external applied magnetic field is increased. It occurs above a characteristic magnetic field value for which the ions become magnetized in the expansion chamber. The hollow density formation is independent of the location of geometric expansion and also on the presence of a radial electric field. The density profile in the source chamber behind the nozzle, however, remains peaked on-axis irrespective of the magnetic field. The electron temperature there, is observed to be hollow and this characteristics continues to the expansion chamber along the field lines. Rotation of the tail electrons in the azimuthal direction due to the gradient-B drift in the expansion chamber leads to an additional off-axis ionization and forms the hollow density profile there. It is shown that, if the ions are not magnetized, then off-axially produced additional plasma is not confined and the density profile retains the on-axis peak nature. The present work demonstrates how the knowledge of the ion magnetization together with tail electrons significantly contributes to the design of an efficient helicon plasma based thruster.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.32
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