1978
DOI: 10.1038/272017a0
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High-β tokamaks?

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Cited by 158 publications
(310 citation statements)
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“…Plasmas are confined in tokamaks by magnetic field lines on nested axisymmetric toroidal magnetic surfaces. 1 This occurs for both conventional tokamaks, with an inductive plasma current density with a maximum at the centre, 1 and in tokamaks with a non-inductive current density with a maximum outside the centre, as presently in JET 2,3 and predicted in the forthcoming ITER. 4 However, some advanced confinement regimes with non inductive currents develop a radial hollow current profile, with a central hole where the current density is almost zero or even negative.…”
mentioning
confidence: 77%
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“…Plasmas are confined in tokamaks by magnetic field lines on nested axisymmetric toroidal magnetic surfaces. 1 This occurs for both conventional tokamaks, with an inductive plasma current density with a maximum at the centre, 1 and in tokamaks with a non-inductive current density with a maximum outside the centre, as presently in JET 2,3 and predicted in the forthcoming ITER. 4 However, some advanced confinement regimes with non inductive currents develop a radial hollow current profile, with a central hole where the current density is almost zero or even negative.…”
mentioning
confidence: 77%
“…This expansion has some peculiarities due to the considered reversed current density. Namely, we consider the expansion for w 0 ðr t Þ up to the second order approximation and the expansion for w 1 …”
Section: Phys Plasmas 18 082508 (2011)mentioning
confidence: 99%
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“…with the resistivity factor N ðZ eff Þ [3]. The term C M is much smaller than C I and can be neglected for the following considerations.…”
Section: à0:73mentioning
confidence: 99%
“…This process takes place in the current sheet formed at the boundary between opposed magnetic fields and is thought to play an important role in space phenomena, such as solar flares 4 and at Earth's magnetosphere 5 , as well as in fusion experiments 6,7 . Despite intense research on the topic over the last decades and a vast quantity of information obtained through space observations 8,9 , numerical simulations 10,11 and experiments [12][13][14][15][16][17][18][19] , the underlying processes of magnetic reconnection are still not fully understood.…”
Section: Introductionmentioning
confidence: 99%