Configurational Effects on Alfvenic modes and Confinement in the H-1NF Heliac

Details Configurational Effects on Alfvenic modes and Confinement in the H-1NF Heliac Configurational Effects on Alfvenic modes and Confinement in the H-1NF Heliac

2009-02-27

arxiv.org/abs/0902.4728v1

Physics

Plasma Physics

Expanded form of paper Ex/P9-11 presented at the 22nd IAEA Fusion Energy Conference, Geneva, Switzerland, 2008, and submitted

Scientific paper

The flexible Heliac coil set of helical axis stellarator H-1 (R=1m, ~0.15-0.2 m) permits access to a wide range of magnetic configurations. Surprisingly, in the absence of any obvious population of energetic particles, Alfven modes normally associated with energetic populations in larger fusion experiments are observed. Using H-1's unique combination of flexibility and advanced diagnostics, RF-generated plasma in H-1 is shown to have a very complex dependence on configuration of both the electron density and fluctuations in the MHD Alfven range. Magnetic fluctuations range from highly coherent, often multi-frequency, to approaching broad-band (df/f ~ 0.02-0.5), in the range 1-200 kHz. Application of datamining techniques to a wide range of configurations classifies these fluctuations and extracts poloidal and toroidal mode numbers, revealing that a significant class of fluctuations exhibit scaling which is i) Alfvenic with electron density (within a constant factor) and ii) shear Alfvenic in rotational transform. This is confirmed by scans within a single pulse, which can follow mode conversions. An array of optical and interferometric diagnostics is combined with the magnetic probe arrays to provide initial information on the internal structure of the MHD modes, and associated 3D effects. The configurational dependence is closely related to the presence of low order rational surfaces; density falls to very low values near, but not precisely at these rational values. Results from a uniquely accurate magnetic field mapping system, combined with a comprehensive model of the vacuum magnetic field in H-1 show that magnetic islands should not dominate the confinement of the configuration, and indicate that the dependence of density on configuration may be attributable to plasma generation effects.

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