Abstract
A comprehensive description of methods, suitable for solving the kinetic equation for fast ions and impurity species in tokamak plasmas using a Monte Carlo approach, is presented. The described methods include Hamiltonian orbit-following in particle and guiding center phase space, test particle or guiding center solution of the kinetic equation applying stochastic differential equations in the presence of Coulomb collisions, neoclassical tearing modes and Alfvén eigenmodes as electromagnetic perturbations relevant to fast ions, together with plasma flow and atomic reactions relevant to impurity studies. Applying the methods, a complete reimplementation of the well-established minority species code ASCOT is carried out as a response both to the increase in computing power during the last twenty years and to the weakly structured growth of the code, which has made implementation of additional models impractical. Also, a benchmark between the previous code and the reimplementation is accomplished, showing good agreement between the codes.
| Original language | English |
|---|---|
| Pages (from-to) | 1310-1321 |
| Number of pages | 12 |
| Journal | Computer Physics Communications |
| Volume | 185 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - Apr 2014 |
| MoE publication type | A1 Journal article-refereed |
Funding
This work was partially funded by the Academy of Finland project No. 259675 and was carried out using the HELIOS supercomputer system at International Fusion Energy Research Centre, Aomori, Japan, under the Broader Approach collaboration between Euratom and Japan, implemented by Fusion for Energy and JAEA. Also the resources of HPC-FF are greatly acknowledged. This work, supported by the European Communities under the contract of Association between Euratom and Tekes, was carried out within the framework of the European Fusion Development Agreement. The views and opinions expressed herein do not necessarily reflect those of the European Commission.
Keywords
- Fast ions
- Impurity tracing
- Monte Carlo
- Orbit-following
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