Copertina

The Energy-Duration Relationship in Astrophysical Self-Organized Criticality Systems

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Aschwanden, Markus J., Araujo, Alexandre
Natura:	Preprint
Pubblicazione:	2026
Soggetti:	Solar and Stellar Astrophysics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

New Trends in Astrophysical Self-Organized Criticality
di: Aschwanden, Markus J.
Pubblicazione: (2025)

Self-Organized Criticality Across Thirteen Orders of Magnitude in the Solar-Stellar Connection
di: Aschwanden, Markus J., et al.
Pubblicazione: (2025)

How the Solar Dynamics Observatory Revolutionized our Physical Understanding of the Sun
di: Aschwanden, Markus J.
Pubblicazione: (2025)

Power Laws Associated with Self-Organized Criticality: A Comparison of Empirical Data with Model Predictions
di: Aschwanden, Markus J., et al.
Pubblicazione: (2025)

Astrophysical Properties of the Sirius Binary System Modeled with MESA
di: Khan, Momin Y., et al.
Pubblicazione: (2024)

Flare Impulsive-phase Durations
di: Dennis, Brian R., et al.
Pubblicazione: (2026)

Astrophysical parameters of LS 437 and the nature of X0726-260
di: Negueruela, Ignacio, et al.
Pubblicazione: (2026)

Placing the Solar System in its Astrophysical Context
di: Gonzalez, Guillermo
Pubblicazione: (2025)

The Role of Long Period Variable Stars in Observational Astrophysics
di: Skowron, Dorota M., et al.
Pubblicazione: (2026)

The r-Process: History, Required Conditions, Astrophysical Sites, and Observations
di: Thielemann, Friedrich-Karl, et al.
Pubblicazione: (2026)

The Longest Duration SGRE Event in Solar Cycle 25
di: Gopalswamy, Nat, et al.
Pubblicazione: (2025)

Analysis of the Stellar Occultations During the Unprecedented Long-Duration Flare
di: Bicz, Kamil, et al.
Pubblicazione: (2024)

The Status of the Astrophysical Parameters of Upper Main Sequence Stars
di: Kueß, Lukas, et al.
Pubblicazione: (2025)

Astrophysical parameters associated to 'hot' stars in Gaia DR3
di: Frémat, Yves
Pubblicazione: (2024)

Bayesian Smooth-Fit Extrapolation of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Astrophysical $S$ Factor
di: Mukhamedzhanov, A. M.
Pubblicazione: (2025)

Hydrogen recombination continuum as the radiative model for stellar optical flares
di: Simões, Paulo J. A., et al.
Pubblicazione: (2024)

Proton-to-Alpha Branching Ratio in the $^{12}$C+$^{12}$C fusion reaction at Astrophysical Energies
di: Yang, Ruojun, et al.
Pubblicazione: (2026)

Stellar Population Astrophysics (SPA) with TNG, Fluorine abundances in seven open clusters
di: Seshashayana, Shilpa Bijavara, et al.
Pubblicazione: (2024)

Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps
di: Hernandez, David, et al.
Pubblicazione: (2025)

Long-Duration Nonthermal Motions in the Supra-Arcade and Loop-Top Region During an Eruptive Solar Flare
di: Gou, Tingyu, et al.
Pubblicazione: (2025)

Universal Constants and Energy Integral in Self-Organized Criticality Systems
di: Aschwanden, Markus
Pubblicazione: (2024)

Stellar Population Astrophysics (SPA) with the TNG: NLTE atmospheric parameters and abundances of giant stars in 33 Open Clusters
di: Ponte, M. Dal, et al.
Pubblicazione: (2025)

The Critical Mass Ratio for W UMa-type Contact Binary Systems
di: Arbutina, Bojan, et al.
Pubblicazione: (2024)

Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics
di: Aerts, Conny, et al.
Pubblicazione: (2023)

Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-Duration Magnetic Field Sector Transition
di: Temmer, Manuela, et al.
Pubblicazione: (2026)

The Digitization of Photographic Spectra in the Dominion Astrophysical Observatory Plate Collection with Commercial Scanners: A Pilot Study
di: Davidge, T. J.
Pubblicazione: (2024)

Skeletal Kinetics Reduction for Astrophysical Reaction Networks
di: Nouri, A. G., et al.
Pubblicazione: (2024)

Relationship Between the Tilt Angle of Sunspot Group and the Properties of the Next Solar Cycle
di: Gao, P. X., et al.
Pubblicazione: (2024)

Stellar Population Astrophysics (SPA) with the TNG 23 IR elemental abundances of 114 giant stars in 41 Open Clusters
di: Seshashayana, Shilpa Bijavara, et al.
Pubblicazione: (2025)

The Components of Cepheid Systems: The FN Vel System
di: Evans, Nancy Remage, et al.
Pubblicazione: (2024)

Habitable Worlds Observatory: The Nature of the Astrophysical r-process
di: Roederer, Ian U., et al.
Pubblicazione: (2025)

Astrophysical aspects of $^{12}$C$(p,γ)^{13}$N reaction
di: Saha, Soumya
Pubblicazione: (2024)

On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona
di: Mondal, Shanwlee Sow, et al.
Pubblicazione: (2025)

Finite-Lens Effect on Self-Lensing in detached White Dwarfs-Main Sequence Binary Systems
di: Sajadian, Sedighe, et al.
Pubblicazione: (2024)

On Benchmarking SRc $α$ Ori using Period-Luminosity Relationship
di: Capuli, Generich H., et al.
Pubblicazione: (2023)

The Relationship between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
di: Victor-French, Kelly, et al.
Pubblicazione: (2025)

Apparent motion of penumbral grains in a sunspot simulation
di: Sobotka, Michal, et al.
Pubblicazione: (2025)

On the Relationship between Solar Spicules and Propagating Coronal Disturbances: The Role of Shocks
di: Chaurasiya, Ravi, et al.
Pubblicazione: (2026)

Fundamentals of Stars: Critical Looks at Mass-Luminosity Relations and Beyond
di: Eker, Z., et al.
Pubblicazione: (2024)

Fast Pulsars, Neutron Stars, and Astrophysical Strange Quark Matter Objects
di: Farrell, Delaney, et al.
Pubblicazione: (2024)