On Solving the Coronal Heating Problem

Abstract

This article assesses the current state of understanding of coronal heating, outlines the key elements of a comprehensive strategy for solving the problem, and warns of obstacles that must be overcome along the way.

Accepted by Solar Physics; Published by Solar Physics

References in corpus (12)

• Ionization balance for optically thin plasmas: rate coefficients for all atoms and ions of the elements H to Ni
• An Ab Initio Approach to the Solar Coronal Heating Problem
• The Dynamic Formation of Prominence Condensations
• Magnetic Reconnection: Sweet-Parker Versus Petschek
• Quiet Sun magnetic fields at high spatial resolution
• TRACE-derived temperature and emission measure profiles along long-lived coronal loops: the role of filamentation
• Magnetic properties of photospheric regions having very low magnetic flux
• Cooling Active Region Loops Observed With SXT and TRACE
• Petschek-like Reconnection with Current-driven Anomalous Resistivity and its Application to Solar Flares
• Coronal Seismology and the Propagation of Acoustic Waves Along Coronal Loops
• Emission measure distribution in loops impulsively heated at the foot-points
• Multithermal Analysis of a CDS Coronal Loop

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• A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
• Pre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST
• ALEXIS: Recreating the X-Ray Emission from the Full Solar Disk as a Linear Combination of Discrete Regions in the Extreme Ultraviolet and Soft X-Rays
• Young M dwarfs flare activity model: Towards better exoplanetary atmospheric characterisation
• Signatures of red-shifted footpoints in the quiescent coronal loop system
• Energy conversion rate of an active region transient brightening estimated by a spectroscopic observation of Hinode
• Line Profile Studies of Coronal Active Regions in Fe XII λ195.12 Using Hinode/EIS
• A Novel Optical Design for Wide-Field Imaging in X-ray Astronomy
• Neutron Stars as the Dark Matter detectors
• Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun
• Solar Kaluza-Klein axion search with NEWS-G
• Flows in Enthalpy Based Thermal Evolution of Loops
• Flute and kink instabilities in a dynamically twisted flux tube with anisotropic plasma viscosity
• Multi-scale Energy Release Events in the Quiet Sun: A Possible Source for Coronal Heating
• Plasma Diagnostics From Active Region and Quiet Sun Spectra Observed by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution
• Modelling 3D magnetic networks in a realistic solar atmosphere
• Nature of the energy source powering solar coronal loops driven by nanoflares
• The Sun as an X-ray star V.: A new method to retrieve coronal filling factors
• The Quiet-Sun DEM Under Kappa: Diagnostic Degeneracy and the Failure of the Conductive Closure
• Characterizing Velocity-Space Signatures of Electron Energization in Large-Guide-Field Collisionless Magnetic Reconnection
• An Approximate Bayesian Deep Learning Approach for Uncertainty-aware Differential Emission Measure Estimates in the Solar Corona from the SDO
• X-ray fine structure of a limb solar flare revealed by Insight-HXMT, RHESSI and Fermi
• The Solar Line Emission Dopplerometer project