Alternative Cellular Avalanche Model for Solar Flares
Exploring an alternative cellular avalanche model based on the maximum release of energy during solar flares, this research delves into optimizing models to study the quasi-static evolution of coronal magnetic fields. Through a series of image objects and studies, the study presents various cellular automaton avalanche models and their implications for understanding solar flares and complex behavior in a dynamic system. Key developments and models discussed include those by Lu, Hamilton, Georgoulis, Vlahos, Norman, Strugarek, Charbonneau, Joseph, and Pirot, shedding light on the deterministically-driven model and its significance.
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An alternative cellular avalanche model based on maximum release of energy during solar flares Nastaran Farhang Hossein Safari & Michael S. Weatland University of Zanjan January 2017
Solar Flares Cellular Automaton Avalanche Models The Optimized Model What is next ? Solar Flares
Solar Flares Cellular Automaton Avalanche Models The Optimized Model What is next ?
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? Cellular Automaton Avalanche Models Studying the quasi-static evolution of coronal magnetic field and their complex behavior by dividing avalanches into discrete elements. Sand-pile Model
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? CA MODELS Development Lu & Hamilton 1991 Georgoulis & Vlahos 1996 Norman et al 2001 Strugarek & Charbonneau The Optimized Model 2014 2017 1. Strugarek, A. & Charbonneau, P. 2014, SoPh, 289, 4137 2. Strugarek, A., Charbonneau, P., Joseph, R. & Pirot, D.,2014, SoPh, 289, 2993
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? Lu & Hamilton Model (1991) 1. Lu, E. T. & Hamilton, R. J. 1991, ApJ, 380, L89 2. Lu, E. T., Hamilton, R. J., McTiernan, J. M., & Bromund, K. R. 1993, ApJ, 412, 841
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? Lu & Hamilton Model (1991) 1. Lu, E. T. & Hamilton, R. J. 1991, ApJ, 380, L89 2. Lu, E. T., Hamilton, R. J., McTiernan, J. M., & Bromund, K. R. 1993, ApJ, 412, 841
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? The Deterministically Driven Model 1. Strugarek, A. & Charbonneau, P. 2014, SoPh, 289, 4137 2. Strugarek, A., Charbonneau, P., Joseph, R. & Pirot, D.,2014, SoPh, 289, 2993
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ? The Deterministically Driven Model 1. Strugarek, A. & Charbonneau, P. 2014, SoPh, 289, 4137 2. Strugarek, A., Charbonneau, P., Joseph, R. & Pirot, D.,2014, SoPh, 289, 2993
Cellular Automaton Avalanche Models The Optimized Model Solar Flares What is next ?
The Optimized Model Solar Flares Cellular Automaton Avalanche Models What is next ? The Optimized Model
The Optimized Model Solar Flares Cellular Automaton Avalanche Models What is next ? The Optimized Model 1. Lu, E. T. & Hamilton, R. J. 1991, ApJ, 380, L89 2. Strugarek, A., Charbonneau, P., Joseph, R. & Pirot, D.,2014, SoPh, 289, 2993
The Optimized Model Solar Flares Cellular Automaton Avalanche Models What is next ? The Optimized Model
The Optimized Model Solar Flares Cellular Automaton Avalanche Models What is next ? The Optimized Model
What is next ? Solar Flares Cellular Automaton Avalanche Models The Optimized Model What is the next step?
