2009
DOI: 10.1016/j.jnucmat.2009.01.232
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Measurement of lower hybrid hot spots using a retarding field analyzer in Tore Supra

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Cited by 26 publications
(43 citation statements)
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“…By varying the launcher position, (retracting it away from a starting position close to the plasma, (see Fig.6e)), such that the radial distance between the field lines (generating the hot spots on the dump plates) and the launcher was increased from 0 to 3.5cm, it was possible to diagnose the radial width of the absorption layer in front of the launcher. This is in agreement with recent observations on Tore Supra [22], but not with the standard modelling of the linear damping of LH waves in the SOL that predicts a dissipation layer of a few mm. This is in agreement with recent observations on Tore Supra [22], but not with the standard modelling of the linear damping of LH waves in the SOL that predicts a dissipation layer of a few mm.…”
Section: Characterisation Of Lh Power Losses In Front Of the Launchersupporting
confidence: 89%
“…By varying the launcher position, (retracting it away from a starting position close to the plasma, (see Fig.6e)), such that the radial distance between the field lines (generating the hot spots on the dump plates) and the launcher was increased from 0 to 3.5cm, it was possible to diagnose the radial width of the absorption layer in front of the launcher. This is in agreement with recent observations on Tore Supra [22], but not with the standard modelling of the linear damping of LH waves in the SOL that predicts a dissipation layer of a few mm. This is in agreement with recent observations on Tore Supra [22], but not with the standard modelling of the linear damping of LH waves in the SOL that predicts a dissipation layer of a few mm.…”
Section: Characterisation Of Lh Power Losses In Front Of the Launchersupporting
confidence: 89%
“…This result is consistent with the low diffusion coefficient for fast electrons from the core to the SOL [12]. It appears that the enhancement of  P at lower n // is due to heating of thermal electrons by collisional damping of the LH waves, however, the effect of fast electrons generated locally in the SOL cannot be discarded [13,14].…”
Section: Resultssupporting
confidence: 72%
“…Hotspots on a PFC magnetically connected to the LH launcher were observed before on JET [37], [38], [39] and on other machines [40], [41], [42], [43]. In our study we refer to all areas seen on the IR cameras which are brighter than normal as hotspots.…”
Section: Observation Of Arcs Via a Dedicated Visible Cameramentioning
confidence: 95%