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University of Illinois at Urbana-Champaign

Ion Cyclotron Resonance Heating Induced Transport in Stellarators and Other Asymmetric Toroids

Abstract

dc:description

A Monte Carlo simulation is developed to model minority ion transport and fundamental ion cyclotron resonance heating (ICRH) in asymmetric magnetic field geometries. A discrete event model is used to superimpose resonance heated nonadiabatic changes in an ion's magnetic moment on a Coulomb scattering model that contains the Spitzer coefficients of drag, velocity diffusion, and pitch angle scattering (PAS). Ion drift orbit equations of motion are set in a magnetic flux coordinate system which separate fast motion along the field lines from slow motion across the lines.

Degree

thesis:*
Name thesis:degree_name
Ph.D.
Level thesis:degree_level
Dissertation
Discipline thesis:degree_discipline
Nuclear Engineering
Grantor
University of Illinois at Urbana-Champaign
Year dc:date
2014

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Splitt, Edward Frank

Subjects

dc:subject × 1

Identifiers

dc:identifier.*
Identifier
(UMI)AAI8815426
OAI identifier oai:identifier
oai:www.ideals.illinois.edu:2142/70913

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Splitt, Edward Frank. Ion Cyclotron Resonance Heating Induced Transport in Stellarators and Other Asymmetric Toroids. Dissertation thesis, University of Illinois at Urbana-Champaign, 2014. http://hdl.handle.net/2142/70913