2006Physics of PlasmasRequires access

Improving confinement in quasi-axisymmetric stellarators

Harry E. Mynick, Allen H. Boozer, L. P. Ku

Open publisher page 13 citations

Abstract

The confinement characteristics of some related quasi-axisymmetric stellarator (QA) designs are compared to gain more physical understanding of what causes the differences in their transport. From this, some general rules are found for features of QA magnetic geometries that are deleterious or helpful for confinement.

About this research paper

What this paper is about

The confinement characteristics of some related quasi-axisymmetric stellarator (QA) designs are compared to gain more physical understanding of what causes the differences in their transport. From this, some general rules are found for features of QA magnetic geometries that are deleterious or helpful for confinement.

Why it matters

OpenAlex reports 13 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

The confinement characteristics of some related quasi-axisymmetric stellarator (QA) designs are compared to gain more physical understanding of what causes the differences in their transport. From this, some general rules are found for features of QA magnetic geometries that are deleterious or helpful for confinement.

Key concepts: Stellarator, Physics, Rotational symmetry, Plasma confinement, Plasma, Magnetic confinement fusion, Magnetohydrodynamics, Mechanics

Related papers

Back to paper searchBrowse research topicsOriginal source
Improving confinement in quasi-axisymmetric stellarators — Research Paper | ScholarLens