Heating in Toroidal Plasmas 1978 1979
DOI: 10.1016/b978-1-4832-8384-5.50025-9
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Heating of a Toroidal Plasma by Skin Current

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Cited by 2 publications
(6 citation statements)
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“…The set of TORTUR equilibria are found to be Mercier-unstable in the region around the magnetic axis where the pressure profile is hollow. This is in agreement with experimental observations because such profiles disappear in a few microseconds [14].…”
Section: Discussionsupporting
confidence: 93%
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“…The set of TORTUR equilibria are found to be Mercier-unstable in the region around the magnetic axis where the pressure profile is hollow. This is in agreement with experimental observations because such profiles disappear in a few microseconds [14].…”
Section: Discussionsupporting
confidence: 93%
“…The plasma is stable up to betas of 18% and, when in an experiment the beta decreases owing to loss of energy, the plasma does not enter into an unstable region. The turbulently heated tokamak plasma is Mercierunstable in the centre of the discharge even for small values of beta, in agreement with the experimentally observed disappearance of the hollow pressure profile [14].…”
Section: Introductionsupporting
confidence: 87%
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“…As examples: an initial skin current layer of a few centimeters thickness with enhanced dissipation is found from radial electron temperature measurements as a function of time with Thomson scattering (KOLFSCHOTEN, 1982). The rate of electron heating during the current ramp is anomalously high, concurring with calculations on heating by ion acoustic turbulence (KALFSBEEK, 1978). Also electron cyclotron radiation observatiohs with an ECE spectrometer as well as X-ray measurements indicate the quenching and scattering of initially freely accelerated electron tails.…”
Section: Stage I: Heating During the Current Rampsupporting
confidence: 81%
“…The TORTUR Tokamak was originally designed to study the turbulent heating with an l/e-width of about 2 cm (KALFSBEEK et al, 1975(KALFSBEEK et al, , 1978. Furthermore, the dissipated energy in the skin, W,, is almost exactly equal to the poloidal magnetic skin energy?…”
Section: Stage Iii: the Turbulent Heating Pulsementioning
confidence: 99%