scholarly journals Tokamak elongation – how much is too much? Part 1. Theory

2015 ◽  
Vol 81 (6) ◽  
Author(s):  
J. P. Freidberg ◽  
A. Cerfon ◽  
J. P Lee

In this and the accompanying paper, the problem of the maximally achievable elongation${\it\kappa}$in a tokamak is investigated. The work represents an extension of many earlier studies, which were often focused on determining${\it\kappa}$limits due to (i) natural elongation in a simple applied pure vertical field or (ii) axisymmetric stability in the presence of a perfectly conducting wall. The extension investigated here includes the effect of the vertical stability feedback system which actually sets the maximum practical elongation limit in a real experiment. A basic resistive wall stability parameter,${\it\gamma}{\it\tau}_{w}$, is introduced to model the feedback system which although simple in appearance actually captures the essence of the feedback system. Elongation limits in the presence of feedback are then determined by calculating the maximum${\it\kappa}$against$n=0$resistive wall modes for fixed${\it\gamma}{\it\tau}_{w}$. The results are obtained by means of a general formulation culminating in a variational principle which is particularly amenable to numerical analysis. The principle is valid for arbitrary profiles but simplifies significantly for the Solov’ev profiles, effectively reducing the 2-D stability problem into a 1-D problem. The accompanying paper provides the numerical results and leads to a sharp answer of ‘how much elongation is too much’?

2015 ◽  
Vol 81 (6) ◽  
Author(s):  
V. D. Pustovitov

Plasma stabilization due to a nearby conducting wall can provide access to better performance in some scenarios in tokamaks. This was proved by experiments with an essential gain in${\it\beta}$and demonstrated as a long-lasting effect at sufficiently fast plasma rotation in the DIII-D tokamak (see, for example, Straitet al.,Nucl. Fusion, vol. 43, 2003, pp. 430–440). The rotational stabilization is the central topic of this review, though eventually the mode rotation gains significance. The analysis is based on the first-principle equations describing the energy balance with dissipation in the resistive wall. The method emphasizes derivation of the dispersion relations for the modes which are faster than the conventional resistive wall modes, but slower than the ideal magnetohydrodynamics modes. Both the standard thin wall and ideal-wall approximations are not valid in this range. Here, these are replaced by an approach incorporating the skin effect in the wall. This new element in the stability theory makes the energy sink a nonlinear function of the complex growth rate. An important consequence is that a mode rotating above a critical level can provide a damping effect sufficient for instability suppression. Estimates are given and applications are discussed.


2008 ◽  
Vol 44 (6) ◽  
pp. 1654-1657 ◽  
Author(s):  
R. Albanese ◽  
Y.Q. Liu ◽  
A. Portone ◽  
G. Rubinacci ◽  
F. Villone

2009 ◽  
Vol 49 (12) ◽  
pp. 125003 ◽  
Author(s):  
M. Okabayashi ◽  
I.N. Bogatu ◽  
M.S. Chance ◽  
M.S. Chu ◽  
A.M. Garofalo ◽  
...  

2014 ◽  
Vol 21 (2) ◽  
pp. 022516 ◽  
Author(s):  
V. D. Pustovitov ◽  
V. V. Yanovskiy

2005 ◽  
Vol 45 (4) ◽  
pp. 285-293 ◽  
Author(s):  
M.E Mauel ◽  
J Bialek ◽  
A.H Boozer ◽  
C Cates ◽  
R James ◽  
...  

2014 ◽  
Vol 24 ◽  
pp. 15-24 ◽  
Author(s):  
M. Ariola ◽  
G. De Tommasi ◽  
A. Pironti ◽  
F. Villone

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