Abstract
Numerical results for the three mono-energetic transport coefficients required for a complete neoclassical description of stellarator plasmas have been benchmarked within an international collaboration. These transport coefficients are flux-surface-averaged moments of solutions to the linearized drift kinetic equation which have been determined using field-line-integration techniques, Monte Carlo simulations, a variational method employing Fourier-Legendre test functions and a finite-difference scheme. The benchmarking has been successfully carried out for past, present and future devices which represent different optimization strategies within the extensive configuration space available to stellarators. A qualitative comparison of the results with theoretical expectations for simple model fields is provided. The behaviour of the results for the mono-energetic radial and parallel transport coefficients can be largely understood from such theoretical considerations but the mono-energetic bootstrap current coefficient exhibits characteristics which have not been predicted.
| Original language | English |
|---|---|
| Article number | 076001 |
| Journal | Nuclear Fusion |
| Volume | 51 |
| Issue number | 7 |
| DOIs | |
| State | Published - Jul 2011 |
Fingerprint
Dive into the research topics of 'Benchmarking of the mono-energetic transport coefficients - Results from the International Collaboration on Neoclassical Transport in Stellarators (ICNTS)'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver