Magnetic structures in the explicitly time-dependent nontwist map

被引:0
|
作者
Janosi, Daniel [1 ,2 ]
Horvath, Aniko [1 ]
Edes, Lili [3 ,4 ]
Kovacs, Tamas [3 ,5 ]
机构
[1] Eotvos Lorand Univ, Dept Theoret Phys, Pazmany Peter Setany 1A, H-1117 Budapest, Hungary
[2] HUN REN Inst Earth Phys & Space Sci, Csatka Endre Utca 6-8, H-9400 Sopron, Hungary
[3] Eotvos Lorand Univ, Dept Atom Phys, Pazmany Peter Setany 1A, H-1117 Budapest, Hungary
[4] Ecole Polytech Fed Lausanne EPFL, Swiss Plasma Ctr SPC, CH-1015 Lausanne, Switzerland
[5] HUN REN ELTE Extragalact Astrophys Res Grp, Pazmany Peter Setany 1A, H-1117 Budapest, Hungary
关键词
SNAPSHOT ATTRACTORS; TRANSPORT; BEHAVIOR; TRANSITION; PARTICLES; LIMITER; FIELDS;
D O I
10.1063/5.0231530
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
We investigate how the magnetic structures of the plasma change in a large aspect ratio tokamak perturbed by an ergodic magnetic limiter, when a system parameter is non-adiabatically varied in time. We model such a scenario by considering the Ullmann-Caldas nontwist map, where we introduce an explicit time-dependence to the ratio of the limiter and plasma currents. We apply the tools developed recently in the field of chaotic Hamiltonian systems subjected to parameter drift. Namely, we follow trajectory ensembles initially forming Kolmogorov Arnold Moser (KAM) tori and island chains in the autonomous configuration space. With a varying parameter, these ensembles, called snapshot tori, develop time-dependent shapes. An analysis of the time evolution of the average distance of point pairs in such an ensemble reveals that snapshot tori go through a transition to chaos, with a positive Lyapunov exponent. We find empirical power-law relationships between both the Lyapunov exponent and the beginning of the transition to chaos (the so-called critical instant), as a function of the rate of the parameter drift, with the former showing an increasing trend and the latter a decreasing trend. We conclude that, in general, coherent tori and magnetic islands tend to break up and become chaotic as the perturbation increases, similar to the case of subsequent constant perturbations. However, because of the continuous drift, some structures can persist longer and exist even at perturbation values where they would not be observable in the constant perturbation case.
引用
收藏
页数:9
相关论文
共 50 条
  • [1] ROBERTSON FORMALISM WITH EXPLICITLY TIME-DEPENDENT OBSERVABLES
    HOLZER, D
    FICK, E
    PHYSICA A, 1990, 168 (02): : 867 - 880
  • [2] Explicitly Solvable Time-dependent Generalized Harmonic Oscillator
    Shi Chang-Guang
    Minoru, Hirayama
    APPLIED MATHEMATICS & INFORMATION SCIENCES, 2012, 6 : 143 - 146
  • [4] The effect of time-dependent γ-pumping on buoyant magnetic structures
    Ali, Abrar A.
    Silvers, Lara J.
    GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS, 2018, 112 (06): : 414 - 430
  • [5] A Chebychev propagator with iterative time ordering for explicitly time-dependent Hamiltonians
    Ndong, Mamadou
    Tal-Ezer, Hillel
    Kosloff, Ronnie
    Koch, Christiane P.
    JOURNAL OF CHEMICAL PHYSICS, 2010, 132 (06):
  • [6] Accurate time propagation for the Schrodinger equation with an explicitly time-dependent Hamiltonian
    Kormann, Katharina
    Holmgren, Sverker
    Karlsson, Hans O.
    JOURNAL OF CHEMICAL PHYSICS, 2008, 128 (18):
  • [7] EXPLICITLY TIME-DEPENDENT COORDINATE TRANSFORMATIONS AND GAUGE-INVARIANCE
    TAKAYA, Y
    PROGRESS OF THEORETICAL PHYSICS, 1976, 55 (06): : 2030 - 2031
  • [8] Numerical modelling of explicitly time-dependent quantum systems with δ-potentials
    Antsiferov, PS
    EUROPEAN JOURNAL OF PHYSICS, 2001, 22 (06) : 623 - 628
  • [9] Transients in a time-dependent logistic map
    Leonel, ED
    da Silva, JKL
    Kamphorst, SO
    PHYSICA A, 2001, 295 (1-2): : 280 - 284
  • [10] PATH-INTEGRAL SOLUTION OF A CLASS OF EXPLICITLY TIME-DEPENDENT POTENTIALS
    GROSCHE, C
    PHYSICS LETTERS A, 1993, 182 (01) : 28 - 36