Speaker
Description
Alpha particles are the key players of a burning plasma as they provide the self-heating required for the sustainment of the fusion burn. At the same time, however, there is only little experimental knowledge on their properties, mostly because of the limited availability of deuterium-tritium (DT) plasmas. Among the challenges that the scientific program of the Joint European Torus (JET) is preparing to face is thus the unambiguous observation of alpha particle physics effects. This encompasses the excitation of alpha-driven Toroidal Alfvén Eigenmodes (TAE) [Ref. 1], as well as the documentation of the general impact of the alpha particles on a number of plasma properties such as, for instance, their expected positive impact on transport through the stabilization of turbulence.
This ambitious scientific goal requires the development of a dedicated scenario at JET, where the production of alpha particles is maximised at limited input power. Of special benefit would here be the capability to produce a steady state supra-thermal deuterium and/or tritium distribution function, as this can in principle maximize the DT reactivity, which is not achieved in a solely thermal plasma. Among the tools that can realize this scenario in DT is an application of the novel ‘3 ion’ scheme [Ref. 2], which is based on ion-cyclotron resonance heating (ICRH) in a mixed species plasma and has recently been applied at JET in D-
In the set of D-
As MeV range ions are produced, the plasma responds in a peculiar way. Despite a dominant electron heating predominantly constrained in the very core region where the IIH layer occurs, we observe T
Another common observation is the presence of a large variety of fast ion driven MHD and, in particular, of Reversed Shear Alfvén Eigenmodes (RSAE), that persist also in the main heating phase, suggesting that a non-monotonic q-profile is unexpectedly achieved.
Furthermore, we have developed a “slowing down” scenario, whereby the NBI source is switched off while ICRH persists (figure 2), as a way to study the decay of the energetic deuteron and fusion born alpha populations. In the “after glow” phase of this discharge there is a spatial change of the alpha particle source (figure 1), which is accompanied by long lived elliptic Alfvén eigenmodes (EAE). Numerical simulations of the drive and damping of these modes are being carried out to establish the contribution of the fusion born alphas to the drive of the observed EAEs, with application to the possibility of developing a new scenario for the destabilization of
We finally discuss the implications of these results for JET DT and ITER, in particular with respect to the facets of alpha particle physics that these plasmas anticipate, what can be learnt from them and their readiness level in view of DT.
Acknowledgements This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 and 2019-2020 under grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission.
References
[Ref. 1] R. Dumont et al. “Scenario preparation for the observation of alpha-driven instabilities and transport of alpha particles in JET DT plasmas”, this conference
[Ref. 2] Y. Kazakov et al., Nature Physics 13, 973–978 (2017)
[Ref. 3] D. Rigamonti et al. Rev. Sci. Instrum. 89, 10I116 (2018)
[Ref. 4] J. Garcia et al. Phys. Plasmas 25, 055902 (2018)
Affiliation | University of Milano-Bicocca |
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Country or International Organization | Italy |