Linear gyrokinetic studies in NCSX, W7-AS, and W7-X stellarators using GS2

Statistics – Computation

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

The GS2 gyrokinetic code is being used to study microinstabilities and turbulence in non-axisymmetric flux-tube geometries. Non-axisymmetric systems, such as stellarators, have a number of interesting features, like natural reversed magnetic shear and a large number of shaping parameters. These offer possibilities for reducing microturbulence and improving performance. The NCSX, W7-AS, and W7-X designs were partially optimized for neoclassical transport; however, the turbulent transport has not been studied in detail. We will present studies of gyrokinetic instabilities in NCSX and W7-X equilibria, including important geometry and linear benchmarks between GS2 and GENE, a gyrokinetic code from IPP. Specifically, we have investigated effects of plasma beta and magnetic shear on linear instabilities in NCSX geometry. In addition, we have conducted studies of the microstability of realistic W7-AS plasmas. Finally, we will discuss improvements to the GS2 trapped particle treatment and a new computational grid generator for GS2. This work was supported by the SciDAC Center for the Study of Plasma Microturbulence and Department of Energy Contract DE-AC02-09CH11466.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Linear gyrokinetic studies in NCSX, W7-AS, and W7-X stellarators using GS2 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Linear gyrokinetic studies in NCSX, W7-AS, and W7-X stellarators using GS2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Linear gyrokinetic studies in NCSX, W7-AS, and W7-X stellarators using GS2 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1368146

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.