25 Years of Self-Organized Criticality: Numerical Detection Methods
arXiv:1506.08142 · doi:10.1007/s11214-015-0158-7
Abstract
The detection and characterization of self-organized criticality (SOC), in both real and simulated data, has undergone many significant revisions over the past 25 years. The explosive advances in the many numerical methods available for detecting, discriminating, and ultimately testing, SOC have played a critical role in developing our understanding of how systems experience and exhibit SOC. In this article, methods of detecting SOC are reviewed; from correlations to complexity to critical quantities. A description of the basic autocorrelation method leads into a detailed analysis of application-oriented methods developed in the last 25 years. In the second half of this manuscript space-based, time-based and spatial-temporal methods are reviewed and the prevalence of power laws in nature is described, with an emphasis on event detection and characterization. The search for numerical methods to clearly and unambiguously detect SOC in data often leads us outside the comfort zone of our own disciplines - the answers to these questions are often obtained by studying the advances made in other fields of study. In addition, numerical detection methods often provide the optimum link between simulations and experiments in scientific research. We seek to explore this boundary where the rubber meets the road, to review this expanding field of research of numerical detection of SOC systems over the past 25 years, and to iterate forwards so as to provide some foresight and guidance into developing breakthroughs in this subject over the next quarter of a century.
arXiv commentSpace Science Review series on SOC
References in corpus (46)
- Power-law distributions in empirical data
- Power laws, Pareto distributions and Zipf's law
- Non-Perturbative Renormalization Flow in Quantum Field Theory and Statistical Physics
- Solar System Objects Observed in the SDSS Commissioning Data
- Power Laws in Solar Flares: Self-Organized Criticality or Turbulence?
- Universal scaling behavior of non-equilibrium phase transitions
- 25 Years of Self-Organized Criticality: Solar and Astrophysics
- Critical Exponents of the Classical 3D Heisenberg Model: A Single-Cluster Monte Carlo Study
- Avalanche and spreading exponents in systems with absorbing states
- A Bayesian test for periodic signals in red noise
- Transport in Sand Piles, Interface Depinning, and Earthquake Models
- The Origin of the Solar Flare Waiting-Time Distribution
- Scaling Approach to Calculate Critical Exponents in Anomalous Surface Roughening
- Nonlinear force-free modeling of the solar coronal magnetic field
- Automated Solar Flare Statistics in Soft X-rays over 37 Years of GOES Observations - The Invariance of Self-Organized Criticality during Three Solar Cycles
- Energy Distribution of Micro-events in the Quiet Solar Corona
- Solar Magnetic Tracking. I. Software Comparison and Recommended Practices
- Universal finite-size scaling behavior and universal dynamical scaling behavior of absorbing phase transitions with a conserved field
- Reconciliation of Waiting Time Statistics of Solar Flares Observed in Hard X-Rays
- A Macroscopic Description of a Generalized Self-Organized Criticality System: Astrophysical Applications
- Coexistence of Self-Organized Criticality and Intermittent Turbulence in the Solar Corona
- Long-period intensity pulsations in the solar corona during activity cycle 23
- Are Solar Active Regions with Major Flares More Fractal, Multifractal, or Turbulent than Others?
- Turbulence, Complexity, and Solar Flares
- An ALMA Disk Mass for the Candidate Protoplanetary Companion to FW Tau
- Intermittency Spectra of the Magnetic Field in Solar Active Regions
- Coronal Fourier power spectra: implications for coronal seismology and coronal heating
- Evidence of Shock-Driven Turbulence in the Solar Chromosphere
- Observations of Dissipation of Slow Magneto-acoustic Waves in a Polar Coronal Hole
- Characterising Complexity in Solar Magnetogram Data using a Wavelet-based Segmentation Method
- The Oslo rice pile model is a quenched Edwards-Wilkinson equation
- Multi-Wavelength Observations of the Spatio-Temporal Evolution of Solar Flares with AIA/SDO: II. Hydrodynamic Scaling Laws and Thermal Energies
- On the scaling of probability density functions with apparent power-law exponents less than unity
- Influence of the definition of dissipative events on their statistics
- The Spatio-Temporal Evolution of Solar Flares Observed with AIA/SDO: Fractal Diffusion, Sub-Diffusion, or Logistic Growth ?
- How to discriminate easily between Directed-percolation and Manna scaling
- Simulating Flaring Events in Complex Active Regions Driven by Observed Magnetograms
- Multi-Wavelength Observations of the Spatio-Temporal Evolution of Solar Flares with AIA/SDO: I. Universal Scaling Laws of Space and Time Parameters
- On the role of self-organised criticality in accretion systems
- A statistical study of SUMER spectral images: events, turbulence, and intermittency
- Exact solution of the totally asymmetric Oslo model
- Drift causes anomalous exponents in growth processes
- Self-organisation to criticality in a system without conservation law
- Properties of Sequential Chromospheric Brightenings and Associated Flare Ribbons
- An Automated Algorithm to Distinguish and Characterize Solar Flares and Associated Sequential Chromospheric Brightenings
- Block scaling in the directed percolation universality class
Cited by in corpus (14)
- 25 Years of Self-Organized Criticality: Solar and Astrophysics
- A Comparison of Flare Forecasting Methods, I: Results from the "All-Clear" Workshop
- 25 Years of Self-Organized Criticality: Concepts and Controversies
- Prediction of Solar Flare Size and Time-to-Flare Using Support Vector Machine Regression
- Significance testing for quasi-periodic pulsations in solar and stellar flares
- Automatic detection of small-scale EUV brightenings observed by the Solar Orbiter/EUI
- Fundamental interactions in self-organized critical dynamics on higher-order networks
- Spectrum of the Stress Dynamics with the Bak-Tang-Wiesenfeld Sandpile
- Inducing Self-Organized Criticality in a network toy model by neighborhood assortativity
- Correlation Functions of Photospheric Magnetic Fields in Solar Active Regions
- Contribution to the Solar Mean Magnetic Field from Different Solar Regions
- Frozen-in Fractals All Around: Inferring the Large Scale Effects of Small-Scale Magnetic Structure
- On the non-Kolmogorov nature of flare-productive solar active regions
- Time path of turbulence and multi-fractality of magnetic field in the evolution of an active region