Heavy impurity transport in the presence of 3D MHD ideal perturbations
Heavy impurity accumulation poses a problem for the operation of tokamaks featuring tungsten plasma facing components.
Early termination of the plasma due to tungsten accumulation is often observed following long
living 3D MHD perturbations. Such scenarios are
often observed in present tokamaks like JET and ASDEX-U, and may be of concern for future
machines like ITER and the European DEMO. Finding a way of designing high performance
scenarios while preventing tungsten accumulation is therefore crucial. This thesis aims at
understanding and modelling heavy impurity transport in tokamak plasmas in the presence
of long living 3D MHD ideal perturbations. In the first part of the thesis, we develop the
theoretical framework to treat the problem, building on stellarator theory for the main ions,
while including the effect of strong toroidal rotation that is only present in tokamaks. The
orderings of the background ion species and the heavy impurity species are developed in
detail. The background ions are subsonic which allows for the calculation of their flows using
the stellarator 1/Μ collisional regime, while the heavy impurities flow supersonically which
requires the inclusion of centrifugal effects for the impurity description. An expression for
the neoclassical heavy impurity flux is obtained which helps identify the contrasting physics
involved. In the second part of the thesis, we present the development of the numerical tools
used to model the problem according to the theoretical framework presented. The usage of
the VMEC code to obtain suitable 3D MHD equilibria is explained. Also, the development of
new codes for calculating the background ion and heat flux flow of the ions, and the impurity
flow from such magnetic equilbria is described. The heavy impurities are followed in this
background plasma using the VENUS-LEVIS code. This code describes the guiding-center
movement of the heavy impurities, accounting for the centrifugal and Coriolis drifts, as well
as for the correct effect of friction and thermal forces exerted by the background ions on
the impurities through a newly implemented collision operator. Finally, the numerical tools
developed in this thesis are used to model the impact of long living 1/1 internal kink modes
on heavy impurity transport. Heavy impurity accumulation is observed to occur rapidly in
the presence of a 1/1 internal kink mode, contrary to what is observed in axisymmetry, in
which off-axis accumulation occurs due to the strong rotation. These cases agree well with
a JET pulse where tungsten accumulates following rapid growth of a continuous 1/1 mode.
In the weakly 3D phase of the pulse, off-axis accumulation of tungsten is observed, whilst
in the strong 3D phase of the pulse, strong tungsten on-axis accumulation is observed. The
theoretical developments allow us to break down all the relevant physics effects. It is seen that
such on-axis accumulation is due to the synergetic effect of the 1/1 mode, the strong toroidal
rotation and the NTV ambipolar electric field.
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