MHD equilibrium reconstruction in the presence of correlated data

2006 ◽  
Vol 46 (2) ◽  
pp. 335-349 ◽  
Author(s):  
Christopher S Jones ◽  
John M Finn
2021 ◽  
Vol 16 (0) ◽  
pp. 2402090-2402090
Author(s):  
Kosuke SUZUKI ◽  
Sadayoshi MURAKAMI ◽  
Satoshi OHDACHI ◽  
Hiroshi IDEI ◽  
Kengoh KURODA ◽  
...  

2005 ◽  
Vol 48 (2) ◽  
pp. 968-977 ◽  
Author(s):  
L. L. Lao ◽  
H. E. St. John ◽  
Q. Peng ◽  
J. R. Ferron ◽  
E. J. Strait ◽  
...  

2001 ◽  
Vol 6 (2) ◽  
pp. 15-28 ◽  
Author(s):  
K. Dučinskas ◽  
J. Šaltytė

The problem of classification of the realisation of the stationary univariate Gaussian random field into one of two populations with different means and different factorised covariance matrices is considered. In such a case optimal classification rule in the sense of minimum probability of misclassification is associated with non-linear (quadratic) discriminant function. Unknown means and the covariance matrices of the feature vector components are estimated from spatially correlated training samples using the maximum likelihood approach and assuming spatial correlations to be known. Explicit formula of Bayes error rate and the first-order asymptotic expansion of the expected error rate associated with quadratic plug-in discriminant function are presented. A set of numerical calculations for the spherical spatial correlation function is performed and two different spatial sampling designs are compared.


1985 ◽  
Vol 40 (10) ◽  
pp. 959-967
Author(s):  
A. Salat

The equivalence of magnetic field line equations to a one-dimensional time-dependent Hamiltonian system is used to construct magnetic fields with arbitrary toroidal magnetic surfaces I = const. For this purpose Hamiltonians H which together with their invariants satisfy periodicity constraints have to be known. The choice of H fixes the rotational transform η(I). Arbitrary axisymmetric fields, and nonaxisymmetric fields with constant η(I) are considered in detail.Configurations with coinciding magnetic and current density surfaces are obtained. The approach used is not well suited, however, to satisfying the additional MHD equilibrium condition of constant pressure on magnetic surfaces.


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