Energy Distribution of Heating Processes in the Quiet Solar Corona

doi:10.1086/311474

The Astrophysical Journal Letters

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Säm Krucker and Arnold O. Benz 1998 ApJ 501 L213 doi:10.1086/311474

Energy Distribution of Heating Processes in the Quiet Solar Corona

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Säm Krucker^1,2 and Arnold O. Benz¹

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Abstract References Cited By

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The Astrophysical Journal Letters

The Astrophysical Journal Letters

Energy Distribution of Heating Processes in the Quiet Solar Corona

Hinode Observation of Photospheric Magnetic Activities Triggering X-ray Microflares Around a Well-developed Sunspot

Fluctuating Energy Storage and Nonlinear Cascade in an Inhomogeneous Coronal Loop

Predicting Observational Signatures of Coronal Heating by Alfvén Waves and Nanoflares

RHESSI Microflares with Quiet Microwave Emission

Hydrodynamic Simulation of a Nanoflare-heated Multistrand Solar Atmospheric Loop

RHESSI Microflare Statistics. I. Flare-Finding and Frequency Distributions

RHESSI Microflare Statistics. II. X-Ray Imaging, Spectroscopy, and Energy Distributions

X-Ray Flaring on the dMe Star, Ross 154

Solar Flare Geometries. II. The Volume Fractal Dimension

A Statistical Model of the Inhomogeneous Corona Constrained by Triple-Filter Measurements of Elementary Loop Strands with TRACE

Different Power-Law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections

Statistical Properties of Synthetic Nanoflares

Stellar Activity on the Young Suns of Orion: COUP Observations of K5-7 Pre-Main-Sequence Stars

Modeling a Coronal Loop Heated by Magnetohydrodynamic Turbulence Nanoflares

Particle Acceleration in Multiple Dissipation Regions

Some Like It Hot: The X-Ray Emission of the Giant Star YY Mensae

A Bayesian Approach to Solar Flare Prediction

Are Coronae of Magnetically Active Stars Heated by Flares? III. Analytical Distribution of Superposed Flares

Signatures of a nanoflare heated solar corona

MHD turbulence and the heating of astrophysical plasmas

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Are Coronae of Magnetically Active Stars Heated by Flares? II. Extreme Ultraviolet and X-Ray Flare Statistics and the Differential Emission Measure Distribution

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Statistical Properties of the Energy Release in Emerging and Evolving Active Regions

Correlating Transition Region Explosive Events with Extreme-Ultraviolet Brightenings

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Flare Heating in Stellar Coronae

On the Heating of the Solar Corona and the Acceleration of the Low-Speed Solar Wind by Acoustic Waves Generated in the Corona

Statistics, Morphology, and Energetics of Ellerman Bombs

Nanoflare Statistics from First Principles: Fractal Geometry and Temperature Synthesis

The Peak Flux Distribution of Solar Radio Bursts

Energy Distribution of Microevents in the Quiet Solar Corona

Energetics of Explosive Events Observed with SUMER

Geometric Effects in Avalanche Models of Solar Flares: Implications for Coronal Heating

Solar Hard X-Ray Bursts and Electron Acceleration Down to 8 keV

Waiting-Time Distributions in Lattice Models of Solar Flares

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Comparison of Transient Network Brightenings and Explosive Events in the Solar Transition Region

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Self-organized Criticality from Separator Reconnection in Solar Flares

Scaling Laws for a Nanoflare-Heated Solar Corona

Extreme-Ultraviolet Flare Activity in Late-Type Stars

A Method to Determine the Heating Mechanisms of the Solar Corona

Time Variability of the "Quiet" Sun Observed with TRACE. II. Physical Parameters, Temperature Evolution, and Energetics of Extreme-Ultraviolet Nanoflares

Time Variability of the "Quiet" Sun Observed with TRACE. I. Instrumental Effects, Event Detection, and Discrimination of Extreme-Ultraviolet Microflares

Statistical Analysis of the Energy Distribution of Nanoflares in the Quiet Sun

Implications from Extreme-Ultraviolet Observations for Coronal Heating of Active Stars

The Magnetic Association of Coronal Bright Points

Chromospheric Magnetic Reconnection and Its Possible Relationship to Coronal Heating

An Empirical Model of a Polar Coronal Hole at Solar Minimum

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