Bifurcations in distributed kinetic systems with aperiodic instability

1984 ◽  
Vol 14 (1) ◽  
pp. 67-87 ◽  
Author(s):  
B.A Malomed ◽  
M.I Tribelsky
1970 ◽  
Vol 4 (1) ◽  
pp. 21-41 ◽  
Author(s):  
C. Montes ◽  
J. Coste ◽  
G. Diener

We study the quasifinear relaxation of an aperiodic instability, namely the instability caused by the temperature anisotropy of a collisionless electron plasma in the absence of an external magnetic field. We give a detailed description of the relaxation process and we examine the validity of the quasilinear theory (existence of separate time scales, quasilinearity of the particles' orbits).


Author(s):  
Jae-Kwang Seo ◽  
Han-Ok Kang ◽  
Juhyeon Yoon ◽  
Keung-Koo Kim

Aperiodic (static) flow instability is an instability related to the change of a flow direction in individual steam generating U-shaped channels operating at given pressure difference. The nature of an aperiodic instability is close to a Ledinegg instability [1] related to the presence of multiple flows at the full hydraulic curve of a U-shaped channel. In this paper, the conditions for a reverse flow for a once-through steam generator (OTSG) with U-shaped modular feedwater line (MFL) are studied. From the results of the studies, it is revealed that the change of a flow direction in the MFL is due to the boiling of the feedwater in the downcomer branch of the U-shaped MFL and that multiple flows start in an area of the extremes corresponding to the minimum pressure difference of the hydraulic curves. Calculation models for predicting a threshold of an aperiodic instability for the OTSG of interest is proposed and the analysis results are compared with the experimental data.


1976 ◽  
Vol 12 (5) ◽  
pp. 696-698
Author(s):  
Yu. A. Gostintsev ◽  
V. N. Marshakov ◽  
L. A. Sukhanov ◽  
P. I. Lebedev

2000 ◽  
Vol 177 ◽  
pp. 465-468
Author(s):  
Irakli S. Nanobashvili

AbstractSome aspects of relativistic electron-positron plasma dynamics in the pulsar magnetosphere are discussed. Namely it is shown that if we take into account the influence of centrifugal force, this gives rise to the new dynamical effect of plasma particle radial braking in the pulsar magnetosphere. Also the possibility of aperiodic instability development in the pulsar magnetosphere is demonstrated. The mechanism for the toroidal magnetic field generation is proposed. Besides, the possible changes of the pulsar magnetosphere structure caused by above mentioned processes is considered.


Author(s):  
Rodrigo A. López ◽  
Marian Lazar ◽  
Shaaban Mohammed Shaaban ◽  
Stefaan Poedts ◽  
Pablo Sebastian Moya

2006 ◽  
Vol 37 (3) ◽  
pp. 625-629 ◽  
Author(s):  
T. Siversky ◽  
Yu. Voitenko ◽  
M. Goossens

1998 ◽  
Vol 34 (5) ◽  
pp. 502-507
Author(s):  
A. M. Grishin ◽  
E. E. Zelenskii

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