kim eun jin


By using a non-perturbative statistical theory (instantons), the PDF tails of

The three forces considered are f 0 = sin(πx)/π and f ± = sin(πx)/π ± sin(2πx)/2π, with f − chosen to be particularly flat (locally cubic) at the equilibrium point x = 0, and f + particularly flat at the unstable fixed po... We consider the classical double-well model of stochastic resonance, in which a particle in a potential V(x,t)=[−x ² ∕2+x ⁴ ∕4−Asin(ωt)x] is subject to an additional stochastic forcing that causes it to occasionally jump between the two wells at x≈±1. Kim Taehyung playing together with his little brothers. Join Facebook to connect with Kim Eun Jin and others you may know. We calculate time-dependent probability density functions (PDFs) for different values of the correlation time and am... We propose a new methodology to understand a stochastic process from the perspective of information geometry by investigating power-law scaling and fractals in the evolution of information. governing the evolution of shear flows. However, these two instabilities often occur simultaneously, with the overlap of the dynamics on a broad range of spatial scales. [1], https://en.wikipedia.org/w/index.php?title=Kim_Eun-jin&oldid=958116601, Olympic field hockey players of South Korea, Field hockey players at the 2000 Summer Olympics, South Korean field hockey biography stubs, Short description is different from Wikidata, Creative Commons Attribution-ShareAlike License, This page was last edited on 22 May 2020, at 01:11.

He has one older brother whose name is not revealed to the public. Explaining how this rotation of solar-type stars evolves in time is currently an interesting but difficult problem in astrophysics. The latter is known to exist in helical turbulence, which is envisioned to arise due to both rotation and convection in solar-type stars. 178, 69-78 (1999). Due to our privacy policy, only current members can send messages to people on ResearchGate. Centro Investigaciones Energéticas, Medioambientales y Tecnológicas, Fluid and Complex Systems Research Centre, Professor of Applied Mathematics and Physics, University of Texas Health Science Center at Houston, Departments of Astronomy & Astrophysics and Physics and Harris School of Public Policy, Center for Astrophysics and Space Sciences (CASS), Physics Department, Time-dependent probability density functions and information diagnostics in forward and backward processes in a stochastic prey-predator model of fusion plasmas, Mechano-electric effect and a heart assist device in the synergistic model of cardiac function, Time-dependent probability density functions and information geometry of the low-to-high confinement transition in fusion plasma, Time-dependent Probability Density Functions and Information Geometry in the Fusion L-H Transition, mathematics Information Length as a Useful Index to Understand Variability in the Global Circulation, Elucidating plasma dynamics in Hasegawa–Wakatani turbulence by information geometry, Information length as a useful index to understand variability in the global circulation, Synergistic Model of Cardiac Function with a Heart Assist Device, Information Length as a New Diagnostic of Stochastic Resonance, Comparing Information Metrics for a Coupled Ornstein–Uhlenbeck Process, Elucidating plasma dynamics in Hasegawa-Wakatani turbulence by information geometry, Entropy Intermittency and Self-Organisation in Turbulence and Statistical Mechanics, Information Geometry of Spatially Periodic Stochastic Systems, Information length as a new diagnostic in the periodically modulated double-well model of stochastic resonance, Intermittency and Self-Organisation in Turbulence and Statistical Mechanics, Information Geometry in a Reduced Model of Self-organised Shear Flows without the Uniform Coloured Noise Approximation, Scalings and fractals in information geometry: Ornstein-Uhlenbeck processes, Scalings and fractals in information geometry: Ornstein–Uhlenbeck processes, Time-Dependent Probability Density Functions and Attractor Structure in Self-Organised Shear Flows, Investigating Information Geometry in Classical and Quantum Systems through Information Length, Information Geometry of Nonlinear Stochastic Systems, Information Geometry in Classical and Quantum Systems, Time-dependent probability density functions and information geometry in stochastic logistic and Gompertz models, Effect of enhanced dissipation by shear flows on transient relaxation and probability density function in two dimensions, Effects of shear flows on the evolution of fluctuations in interchange turbulence, Far-From-Equilibrium Time Evolution between Two Gamma Distributions, Far-from-Equilibrium Time Evolution between two Gamma Distributions, Geometric structure and information change in phase transitions, Information Geometry of Non-Equilibrium Processes in a Bistable System with a Cubic Damping, Geometrical structure in phase transition, Absolute versus convective helical magnetorotational instabilities in Taylor-Couette flows, Signature of nonlinear damping in geometric structure of a nonequilibrium process, Dynamical model for spindown of solar-type stars, Time-dependent probability density function in cubic stochastic processes, Study of improved confinement by a stepwise increase of the input heating power for tokamak plasmas, Suppression of a laminar kinematic dynamo by a prescribed large-scale shear, Sustainable theory of a logistic model - Fisher Information approach, Structures in Sound: Analysis of Classical Music Using the Information Length, Geometric structure and geodesic in a solvable model of nonequilibrium process, Suppression of a kinematic dynamo by large shear, Novel mapping in non-equilibrium stochastic processes, Geometric method for forming periodic orbits in the Lorenz system, Variability and degradation of homeostasis in self-sustained oscillators, Complementary relations in non-equilibrium stochastic processes, Noise-Driven Phenotypic Heterogeneity with Finite Correlation Time in Clonal Populations, A Fractional Fokker-Planck Model for Anomalous Diffusion, Investigation of the statistical distance to reach stationary distributions, Detailed mathematical and numerical analysis of a dynamo model, SI - Network of mutually repressive metastasis regulators can promote cell heterogeneity and metastatic transitions, Network of mutually repressive metastasis regulators can promote cell heterogeneity and metastatic transitions, Oscillatory control parameters in nonlinear chaotic systems, Confinement improvement by fluctuating input power, Deciphering interactions of complex systems that do not satisfy detailed balance, On the self-organizing process of large scale shear flows, Dynamic model of dynamo (magnetic activity) and rotation, Effect of stochasticity in mean field dynamo models, Determining the temporal dynamics of the solar α effect, A generic model for transport in turbulent shear flows. Lumped-parameter models combined with pressure-volume loop analysis are very effective in simulating clinical scenar... Stochastic resonance is a subtle, yet powerful phenomenon in which a noise plays an interesting role of amplifying a signal instead of attenuating it.

Antonio Ferriz-Mas, Astronomical Society of the Pacific Conference Series, Vol. The present letter attempts to analytically calculate the effects of zonal flow suppression of the ITG turbulence through deriving a modified dispersion relation including the back... We present the first prediction of the probability distribution function (PDF) for self-organization of shear flows modeled by a nonlinear diffusion equation with a stochastic forcing. In particular, Fisher Information (FI) has been evoked as a useful measure of sustainability and the variability of dynamical systems including self-organising systems. Self-organisation is a novel property of complex systems where ordered collective behaviour emerges on a macroscale, which provides a unifying theory for many systems that are constantly changing in time and space. By consi... We present results from time-dependent hydrodynamic calculations of the interaction between internal gravity waves and the mean radial differential rotation in the solar tachocline. https://www.mdpi.com/journal/entropy/special_issues/stellar. Despite complex nonlinear dynamics, coherent structures such as shear flows often form from small-scale turbulence, which then feed back on small-scales. Using a function, Atanh(t/T) for the transition of inpu... We numerically solve the magnetic induction equation in a spherical shell geometry, with a kinematically prescribed axisymmetric flow that consists of a superposition of a small-scale helical flow and a large-scale shear flow. 91, 185006, 2003) to a stochastic model. A remarkable consequence of this mutual interaction is self-organization, which provides a powerful parad... We present a statistical theory of intermittency in plasma turbulence based on short-lived coherent structures (instantons).

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