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 UP11: Poster Session VIII: MST; DIII-D Tokamak; SPARC, C-Mod, and High Field Tokamaks; HBT-EP; Transport and LPI in ICF Plasmas, Hydrodynamic Instability; HEDP Posters; Space and Astrophysical Plasmas (2:00pm-5:00pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.UP11.144
Abstract: UP11.00144 : Ferrite Based Antennas for Lanching Shear Alfven and Whistler Waves*
Presenter:
Walter N Gekelman
(Univ of California - Los Angeles)
Authors:
Walter N Gekelman
(Univ of California - Los Angeles)
Patrick Pribyl
(Univ. of California, Los Angeles)
Stephen T Vincena
(Univ of California - Los Angeles)
Dennis Papadopoulis
(Univ. Maryland)
Space missions place a premium on efficient low frequency wave antennas. This is especially true for Radiation Belt Remediation (RBR) intended to precipitate “MeV” satellite “killer” electrons injected following High Altitude Nuclear Detonation. Observations supported by analysis place premium on high amplitude whistlers. We have previously suggested1 that inserting a core containing Co-Fe nanoparticles in conventional antennas can increase the radiation resistance by more than 50dB, with negligible hysteresis loss. We conducted proof-of-principle experiments using less efficient ferrite material. Antenna for launching shear Alfvén and whistler waves were tested on the Large Plasma device at UCLA. A shear wave antenna µ=80 launched a wave f/fci = 0.65 with 80 times the amplitude that an identical antenna without a core. Two or more ferrite based antennas have launched shear waves with kperp/kpara = 98. Whistler waves were launched and detected meters away. Different configurations and phasing of the antennas will be presented
1:Papadopoulos et al. COSPAR 2018, Paper C5.1-0017-18
*Funded by a MURI award : Air Force (7479-Z8142001) in collaboration with the U of Maryland. The LAPD is part of the Basic Plasma Science Facility funded by NSF and DOE.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.144
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