Bulletin of the American Physical Society
75th Annual Gaseous Electronics Conference
Volume 67, Number 9
Monday–Friday, October 3–7, 2022;
Sendai International Center, Sendai, Japan
The session times in this program are intended for Japan Standard Time zone in Tokyo, Japan (GMT+9)
Session EM2: Workshop II: Plasma Physics for Space Propulsion Technologies
10:30 AM–5:45 PM,
Monday, October 3, 2022
Sendai International Center
Room: Hagi
Chair: Daisuke Kuwahara, Chubu University
Abstract: EM2.00009 : The Blue Core Paradigm
5:00 PM–5:45 PM
Presenter:
Roderick W Boswell
(Australian Natl University)
Authors:
Roderick W Boswell
(Australian Natl University)
Felicien Filleul
(Te Pu ̄naha A ̄tea - Auckland Space Institute, Department of Engineering Science, The University of Auckland, Auckland, 1010, New Zealand)
Antonella Caldarelli
(Te Pu ̄naha A ̄tea - Auckland Space Institute, Department of Engineering Science, The University of Auckland, Auckland, 1010, New Zealand)
Christine Charles
(Space Plasma, Power and Propulsion Laboratory, NPAA, Research School of Physics, The Australian National University, Canberra, ACT 2601, Australia)
Kazunori Takahashi
(Tohoku University)
Alex Bennet
(Lam Research, Cushing Parkway, Fremont, CA, USA)
Two new experiments have looked at the generation of blue cores without any evidence of helicon waves existing in the discharge. Both experiments share the same physical dimensions and magnetic field topologies but differ in the type of antenna employed and the driving frequency; a double-saddle driven at 13.56 MHz on one-hand, a single loop at 27.12 MHz on the other. In each, a Helmholtz pair of solenoids can be progressively moved away from the antenna to observe the effect on the discharge. Strong ArII emission and densities ≥ 1012 cm−3 are obtained for Prf ≥ 200 W and applied magnetic fields ≥ 600 G, when the Helmholtz pair is placed 30 cm away from the antenna. EEPFs measured along the magnetic field lines crossing the skin-depth region under the loop antenna are bi-Maxwellians with hot electrons in the inelastic energy range up to 50 cm away from the antenna. Plasma potential mappings show a strong ion radial confinement and an axial trapping of the electrons, matching with the location of maximum plasma density and of the blue core.
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