Characterisation oga helicon source for non-linear microwave coupling experiments in a magnetised plasma

Wilson, Kieran J and Selman, Liam and Whyte, Colin G and MacInnes, Philip and Young, Alan R and Phelps, Alan R and Cross, Adrian W and Zhang, Liang and Eliasson, Bengt and Speirs, David C and Robertson, Craig W and Ronald, Kevin and Cairns, Robert, Alan and Bingham, Robert and Bamford, Ruth and Koepke, Mark E (2021) Characterisation oga helicon source for non-linear microwave coupling experiments in a magnetised plasma. In: 63rd Annual Meeting of the APS Division of Plasma Physics, 2021-12-08 - 2021-12-12. (https://meetings.aps.org/Meeting/DPP21/Session/TP1...)

[thumbnail of Wilson-etal-APS-2021-Characterisation-oga-helicon-source-for-non-linear-microwave-coupling-experiments-in-a-magnetised-plasma]
Preview
Text. Filename: Wilson_etal_APS_2021_Characterisation_oga_helicon_source_for_non_linear_microwave_coupling_experiments_in_a_magnetised_plasma.pdf
License: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 logo

Download (63kB)| Preview

Abstract

As a non-linear medium, parametric instabilities arise when powerful EM waves propagate in plasma. Such effects are seen in laser-plasma, RF–ionospheric and tokamak heating scenarios. Fusion plasmas in a spherical aspect tokamak are difficult to heat due to their high densities, making the lower cyclotron resonances unreachable via direct means. Beat-wave interactions involving multiple EM waves can be used to excite such resonances. Laser, fusion and ionospheric environments pose diagnostic challenges to fully investigate these processes and measure their impact on macroscopic properties such as density, temperature and energy distributions. For this reason a helicon source driven between 3 & 30 MHz has been commissioned. The 1 m diameter, 3 m long stainless-steel vessel is immersed in a static B-field of up to 90 mT formed by 6 electromagnets. The resulting relatively tenuous (1018 m-3), cool (<10 eV) plasma is ideal for parametric wave coupling experiments with powerful microwave beams. Microwave interferometry, frequency compensated Langmuir and RF pickup probes will diagnose how these processes impact the plasma. This paper presents initial experiments characterising the apparatus, with comparison to numerical simulations. *Supported by UK EPSRC (EP/R004773/1).

ORCID iDs

Wilson, Kieran J, Selman, Liam, Whyte, Colin G ORCID logoORCID: https://orcid.org/0000-0002-5431-2443, MacInnes, Philip ORCID logoORCID: https://orcid.org/0000-0003-2882-9817, Young, Alan R ORCID logoORCID: https://orcid.org/0000-0002-3494-1242, Phelps, Alan R ORCID logoORCID: https://orcid.org/0000-0002-1100-1012, Cross, Adrian W ORCID logoORCID: https://orcid.org/0000-0001-7672-1283, Zhang, Liang ORCID logoORCID: https://orcid.org/0000-0002-6317-0395, Eliasson, Bengt ORCID logoORCID: https://orcid.org/0000-0001-6039-1574, Speirs, David C ORCID logoORCID: https://orcid.org/0000-0001-5705-6126, Robertson, Craig W ORCID logoORCID: https://orcid.org/0000-0002-3552-466X, Ronald, Kevin ORCID logoORCID: https://orcid.org/0000-0002-8585-0746, Cairns, Robert, Alan, Bingham, Robert ORCID logoORCID: https://orcid.org/0000-0002-9843-7635, Bamford, Ruth and Koepke, Mark E;