Multiscale self-organized criticality and powerful X-ray flares
arXiv:astro-ph/0311445 · doi:10.1140/epjb/e2003-00304-3
Abstract
A combination of spectral and moments analysis of the continuous X-ray flux data is used to show consistency of statistical properties of the powerful solar flares with 2D BTW prototype model of self-organized criticality.
References in corpus (6)
- Power Laws in Solar Flares: Self-Organized Criticality or Turbulence?
- Multifractal scaling in the Bak-Tang-Wiesenfeld Sandpile and edge events
- Solar Flares as Cascades of Reconnecting Magnetic Loops
- 1/f noise from correlations between avalanches in self-organized criticality
- Turbulent self-organized criticality
- Multiscaling of galactic cosmic ray flux
Cited by in corpus (8)
- 25 Years of Self-Organized Criticality: Solar and Astrophysics
- Inter-occurrence Times in the Bak-Tang-Wiesenfeld Sandpile Model: A Comparison with the Turbulent Statistics of Solar Flares
- Intensity Thresholds and the Statistics of the Temporal Occurrence of Solar Flares
- Precise toppling balance, quenched disorder, and universality for sandpiles
- A Self-Organized-Criticality model consistent with statistical properties of edge turbulence in a fusion plasma
- Macroscopic control parameter for avalanche models for bursty transport
- Directed Fixed Energy Sandpile Model
- Randmoness and Step-like Distribution of Pile Heights in Avalanche Models