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MHD theory predicts that instabilities inside the plasma are stabilized by increasing the "[[Magnetic well|magnetic well]]". This idea is supported by magnetic well scan experiments in TJ-II. | MHD theory predicts that instabilities inside the plasma are stabilized by increasing the "[[Magnetic well|magnetic well]]". This idea is supported by magnetic well scan experiments in TJ-II. | ||
The level of fluctuations, the degree of intermittency and the radial correlation of relevant quantities increase as the magnetic well is reduced. | |||
<ref>[http://dx.doi.org/10.1088/0741-3335/43/12A/324 C. Hidalgo et al, ''On the radial scale of fluctuations in the TJ-II stellarator'', Plasma Phys. Control. Fusion '''43''' (2001) A313-A321]</ref> | <ref>[http://dx.doi.org/10.1088/0741-3335/43/12A/324 C. Hidalgo et al, ''On the radial scale of fluctuations in the TJ-II stellarator'', Plasma Phys. Control. Fusion '''43''' (2001) A313-A321]</ref> | ||
<ref>[http://link.aip.org/link/?PHPAEN/9/713/1 J. Castellano et al, ''Magnetic well and instability thresholds in the TJ-II stellarator'', Phys. Plasmas '''9''' (2002) 713]</ref> | |||
== References == | == References == | ||
<references /> | <references /> |