New Trends in Astrophysical Self-Organized Criticality
Markus J. Aschwanden

TL;DR
This review summarizes recent developments in astrophysical self-organized criticality (SOC) research from 2015 to 2025, covering various cosmic phenomena and systems, highlighting new insights and trends in the field.
Contribution
It provides a comprehensive overview of the latest astrophysical SOC studies, emphasizing recent phenomena and the evolution of understanding over the past decade.
Findings
Identification of new SOC behaviors in solar and stellar phenomena
Insights into SOC mechanisms in planetary and galactic systems
Compilation of recent observational and theoretical advances
Abstract
This review is focused on recent {\sl Self-Organized Criticality (SOC)} literature of astrophysical phenomena, covering the last decade of (2015-2025), while previous SOC literature (1987-2014) is reviewed elsewhere. The selection of literature is mostly based on searches with the NASA-supported {\sl Astrophysics Data System (ADS)}. The discussed astrophysical SOC phenomena are subdivided into solar flares, solar atmosphere (photosphere, chromosphere, corona), heliospheric systems (coronal mass ejections, solar wind, solar energetic particles), planetary systems (asteroids and small bodies, lunar cratering, Saturnian ring systems, magnetospheric systems), stellar flares, and galactic systems (pulsar glitches, gamma ray bursts, soft gamma-ray repeaters, supergiant fast X-ray transients, fast transient radio bursts, magnetars, blazars, black holes).
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