Wave Heating of the Solar Atmosphere
arXiv:1501.06708 · doi:10.1098/rsta.2014.0261
Abstract
Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their significance has increased because of their potential as a remote diagnostic tool and their presumed contribution to plasma heating processes. We discuss our current understanding on coronal heating by magnetic waves, based on recent observational evidence and theoretical advances. The discussion starts with a selection of observational discoveries that have brought magnetic waves to the forefront of the coronal heating discussion. Then, our theoretical understanding on the nature and properties of the observed waves and the physical processes that have been proposed to explain observations are described. Particular attention is given to the sequence of processes that link observed wave characteristics with concealed energy transport, dissipation, and heat conversion. We conclude with a commentary on how the combination of theory and observations should help us understanding and quantifying magnetic wave heating of the solar atmosphere.
Accepted for publication in Royal Society of London Philosophical Transactions Series A
References in corpus (22)
- Bayes in the sky: Bayesian inference and model selection in cosmology
- Alfven Waves in the Lower Solar Atmosphere
- A Contemporary View of Coronal Heating
- Convectively driven vortex flows in the Sun
- Persistent Doppler shift oscillations observed with HINODE/EIS in the solar corona: spectroscopic signatures of Alfvenic waves and recurring upflows
- Nonlinear Instability of kink oscillations due to shear motions
- An Interface Region Imaging Spectrograph first view on Solar Spicules
- On the prevalence of small-scale twist in the solar chromosphere and transition region
- Fine strand-like structure in the solar corona from MHD transverse oscillations
- First direct measurements of transverse waves in solar polar plumes using SDO/AIA
- The Spectroscopic Signature of Quasi-periodic Upflows in Active Region Timeseries
- Resonant absorption in complicated plasma configurations: applications to multi-stranded coronal loop oscillations
- Spectroscopic signature of Alfvén waves damping in a polar coronal hole up to 0.4 solar radii
- Energy flux of Alfven waves in weakly ionized plasma
- Evidence for Wave Heating of the Quiet Sun Corona
- Global coronal seismology
- Synthetic observations of wave propagation in a sunspot umbra
- On the multi-threaded nature of solar spicules
- Observational Signatures of Waves and Flows in the Solar Corona
- The detection of upwardly propagating waves channelling energy from the chromosphere to the low corona
- Determination of the cross-field density structuring in coronal waveguides using the damping of transverse waves
- Bayesian Analysis of Solar Oscillations
Cited by in corpus (64)
- Solar UV and X-Ray Spectral Diagnostics
- Coronal heating by MHD waves
- Partially Ionized Plasmas in Astrophysics
- Recent advances in coronal heating
- MHD Waves in open coronal structures
- Generalized phase mixing: Turbulence-like behaviour from unidirectionally propagating MHD waves
- Measurements of Non-Thermal Line Widths in Solar Active Regions
- Transverse Wave Induced Kelvin-Helmholtz Rolls in Spicules
- Laser-produced magnetic-Rayleigh-Taylor unstable plasma slabs in a 20 T magnetic field
- The Heating of Solar Coronal Loops by Alfven Wave Turbulence
- Investigating `dark' energy in the solar corona using forward modeling of MHD waves
- Excitation of decay-less transverse oscillations of coronal loops by random motions
- Contribution of mode coupling and phase-mixing of Alfvén waves to coronal heating
- Forward Modelling of Standing Slow Modes in Flaring Coronal Loops
- Decayless oscillations in solar coronal bright points
- Energetics of the Kelvin-Helmholtz instability induced by transverse waves in twisted coronal loops
- On Kelvin-Helmholtz and parametric instabilities driven by coronal waves
- Forward Modelling of Standing Kink Modes in Coronal Loops I. Synthetic Views
- On the spatial scales of wave heating in the solar chromosphere
- A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona
- Generating transverse loop oscillations through a steady-flow driver
- Chromospheric Heating by MHD Waves and Instabilities
- Non-linear damping of standing kink waves computed with Elsasser variables
- Multi-fluid Approach to High-frequency Waves in Plasmas. II. Small-amplitude Regime in Partially Ionized Media
- Impulsively Generated Wave Trains in Coronal Structures: I. Effects of Transverse Structuring on Sausage Waves in Pressureless Tubes
- The role of Alfvén wave heating in solar prominences
- High frequency decayless waves with significant energy in Solar Orbiter/EUI observations
- Resonant Absorption of Axisymmetric Modes in Twisted Magnetic Flux Tubes
- Coronal cooling as a result of mixing by the nonlinear Kelvin--Helmholtz instability
- Multi-fluid approach to high-frequency waves in plasmas: I. Small-amplitude regime in fully ionized medium
- Why Does the Solar Corona Abnormally Rotate Faster Than the Photosphere?
- Coronal loop transverse oscillations excited by different driver frequencies
- Model comparison for the density structure across solar coronal waveguides
- Impulsively generated wave trains in coronal structures: II. Effects of transverse structuring on sausage waves in pressureless slabs
- The Magnetic Properties of Heating Events on High-Temperature Active Region Loops
- Damping of slow surface sausage modes in photospheric waveguides
- Properties of Streamer Wave Events Observed During the STEREO Era
- On Mode Conversion, Reflection and Transmission of Magneto-Acoustic Waves from Above in an Isothermal Stratified Atmosphere
- Is It Small-scale Weak Magnetic Activity That Effectively Heats the Upper Solar Atmosphere?
- Revisiting the relation between nonthermal line widths and transverse MHD wave amplitudes
- Spectroscopic evidence of Alfvén wave damping in the off-limb solar corona
- In-situ generation of transverse MHD waves from colliding flows in the solar corona
- Influence of the Lower Atmosphere on Wave Heating and Evaporation in Solar Coronal Loops
- Resonant Damping of Kink Modes in Solar Coronal Slabs
- Damping of slow surface kink modes in solar photospheric waveguides modeled by one-dimensional inhomogeneities
- Simulated interaction of MHD shock waves with a complex network-like region
- Impulsively Generated Kink Wave Trains in Solar Coronal Slabs
- Magnetically coupled atmosphere, fast sausage MHD waves, and forced magnetic field reconnection during the SOL2014-09-10T17:45 flare
- How transverse MHD wave-driven turbulence influences the density filling factor in the solar corona?
- Heating of quiescent coronal loops caused by nearby eruptions observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager
- The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
- A Global Survey of EUV Corona Power Spectra
- Spectroscopic study of solar transition region oscillations in the quiet-Sun observed by IRIS using Si IV spectral line
- Thermal conduction effects on formation of chromospheric solar tadpole-like jets
- Comparison of the Scaling Properties of EUV Intensity Fluctuations in Coronal Hole and Quiet-Sun Regions
- On the nature of transverse coronal waves revealed by wavefront dislocations
- Oblique Quasi-Kink Modes in Solar Coronal Slabs Embedded in an Asymmetric Magnetic Environment: Resonant Damping, Phase and Group Diagrams
- Propagation of Leaky MHD Waves at Discontinuities with Tilted Magnetic Field
- Numerical simulations of the emerging plasma blob into a solar coronal hole
- Global Coronal Magnetic Field Estimation Using Bayesian Inference
- Multi-height probing of horizontal flows in the solar photosphere
- Coronal heating problem solution by means of axion origin photons
- Enhanced Phase Mixing of Torsional Alfvén Waves in Stratified and Divergent Solar Coronal Structures, Paper I: Linear Solutions
- Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH