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From the theoretical perpective we should consider different mechanisms: | From the theoretical perpective we should consider different mechanisms: | ||
The role of phase space driven instabilities <ref>S. Itoh and K. Itoh Scientific Reports 2, 860 (2012)</ref>; role of fast particles on MHD stability <ref>L. Gonzalo et al., Physics of Plasmas 23, 062319 (2016)</ref>; the role of plasma gradient driven instabilities <ref>E. Sánchez et al., Nucl Fusion 59, 076029 (2019)</ref>. | The role of phase space driven instabilities <ref>S. Itoh and K. Itoh Scientific Reports 2, 860 (2012)</ref>; role of fast particles on MHD stability <ref>L. Gonzalo et al., Physics of Plasmas 23, 062319 (2016)</ref>; the role of plasma gradient driven instabilities <ref>E. Sánchez et al., Nucl Fusion 59, 076029 (2019)</ref> and the influence of ECRH in the turbulent drive <ref>X. Wang et al., Nucl Fusion 57, 57, 116046 (2017)</ref>. | ||
From the experimental perspective the goal is the investigation of the influence of ECRH on / off power heating in the dynamics of edge & core fluctuations and transport: 1) Level of fluctuations, 2) Phase relation between density and potential fluctuations, 3) Turbulent ExB transport. | From the experimental perspective the goal is the investigation and characterization of the influence of ECRH on / off power heating in the dynamics of edge & core fluctuations and transport in the TJ-II stellarator, including: 1) Level of fluctuations, 2) Phase relation between density and potential fluctuations, 3) Turbulent ExB transport. | ||
== International or National funding project or entity == | == International or National funding project or entity == |
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