Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
arXiv:1503.01769 · doi:10.1007/s11214-015-0141-3
Abstract
The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool photosphere and the intensely heated transition region and corona. Compressible and incompressible waves propagating through the chromosphere can supply significant amounts of energy to the interface region and corona. In recent years an abundance of high-resolution observations from state-of-the-art facilities have provided new and exciting ways of disentangling the characteristics of oscillatory phenomena propagating through the dynamic chromosphere. Coupled with rapid advancements in magnetohydrodynamic wave theory, we are now in an ideal position to thoroughly investigate the role waves play in supplying energy to sustain chromospheric and coronal heating. Here, we review the recent progress made in characterising, categorising and interpreting oscillations manifesting in the solar chromosphere, with an impetus placed on their intrinsic energetics.
48 pages, 25 figures, accepted into Space Science Reviews
References in corpus (36)
- The Solar Optical Telescope for the Hinode Mission: An Overview
- CRISP Spectropolarimetric Imaging of Penumbral Fine Structure
- Alfven Waves in the Lower Solar Atmosphere
- Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
- Magnetic Landscape of Sun's Polar Region
- Convectively driven vortex flows in the Sun
- The solar chromosphere at high resolution with IBIS. I. New insights from the Ca II 854.2 nm line
- Nonlinear Fast Magnetoacoustic Wave Propagation in the Neighbourhood of a 2D magnetic X-point: Oscillatory Reconnection
- Large amplitude oscillation of a polar crown filament in the pre-eruption phase
- Magnetoacoustic shocks as driver of quiet Sun mottles
- A Chain of Winking (Oscillating) Filaments Triggered by an Invisible Extreme-Ultraviolet Wave
- The Nature of Running Penumbral Waves Revealed
- Observations and Implications of Large-Amplitude Longitudinal Oscillations in a Solar Filament
- Statistical properties of the Disk Counterparts of Type II Spicules from simultaneous observations of RBEs in Ca II 8542 and Hα
- The solar chromosphere at high resolution with IBIS. II. Acoustic shocks in the quiet internetwork and the role of magnetic fields
- Observation of multiple sausage oscillations in cool postflare loop
- Dynamics of the solar magnetic bright points derived from their horizontal motions
- Revision of Solar Spicule Classification
- Propagating intensity disturbances in polar corona as seen from AIA/SDO
- Overdamped Alfven waves due to ion-neutral collisions in the solar chromosphere
- Large-Amplitude Oscillation of an Erupting Filament as Seen in EUV, H-alpha and Microwave Observations
- Transverse oscillations of two coronal loops
- Oscillations in a sunspot with light bridges
- Are Chromospheric Nanoflares a Primary Source of Coronal Plasma?
- High-Frequency Oscillations in a Solar Active Region observed with the Rapid Dual Imager
- High Resolution Observations of Chromospheric Jets in Sunspot Umbra
- DOT Tomography of the Solar Atmosphere VII. Chromospheric Response to Acoustic Events
- Longitudinal oscillations in density stratified and expanding solar waveguides
- The energy of waves in the photosphere and lower chromosphere: III. Inversion setup for Ca II H spectra in local thermal equilibrium
- Observation of standing kink waves in solar spicules
- Solar H-alpha Oscillations from Intensity and Doppler Observations
- Nanoflare Activity in the Solar Chromosphere
- The energy of waves in the photosphere and lower chromosphere: II. Intensity statistics
- Discovery of Spatial Periodicities in a Coronal Loop using Automated Edge-Tracking Algorithms
- Variations of magnetic bright point properties with longitude and latitude as observed by Hinode/SOT G-band data
- Acceleration of Type 2 Spicules in the Solar Chromosphere - 2: Viscous Braking and Upper Bounds on Coronal Energy Input
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- The European Solar Telescope
- A global view of velocity fluctuations in the corona below 1.3 with CoMP
- Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
- The First Ionization Potential Effect from the Ponderomotive Force: On the Polarization and Coronal Origin of the Alfven Waves
- Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI
- Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE): II. Flares and Eruptions
- An Inside Look at Sunspot Oscillations with Higher Azimuthal Wavenumbers
- Coronal Quasi-periodic Fast-mode Propagating Wave Trains
- Vortex Flow Properties in Simulations of Solar Plage Region: Evidence for their role in chromospheric heating
- High Frequency Waves in Chromospheric Spicules
- Preflare very long-periodic pulsations observed in Halpha emission before the onset of a solar flare
- The solar chromosphere at millimetre and ultraviolet wavelengths. I. Radiation temperatures and a detailed comparison
- A Hot Downflowing Model Atmosphere For Umbral Flashes And The Physical Properties Of Their Dark Fibrils
- The Frequency-dependent Damping of Slow Magnetoacoustic Waves in a Sunspot Umbral Atmosphere
- Magnetoacoustic Waves in a Stratified Atmosphere with a Magnetic Null Point
- Observations of solar chromospheric oscillations at 3 mm with ALMA
- Stirring the Base of the Solar Wind: On Heat Transfer and Vortex Formation
- Magnetoacoustic Wave Energy Dissipation in the Atmosphere of Solar Pores
- Why Does the Solar Corona Abnormally Rotate Faster Than the Photosphere?
- Observational study of chromospheric heating by acoustic waves
- Three-dimensional MHD wave propagation near a coronal null point: a new wave mode decomposition approach
- Resonant absorption of surface sausage and surface kink modes under photospheric conditions
- Umbral chromospheric fine structure and umbral flashes modelled as one: the corrugated umbra
- Transition to turbulence in nonuniform coronal loops driven by torsional Alfven waves
- High-frequency wave power observed in the solar chromosphere with IBIS and ALMA
- The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores
- Dynamics of internetwork chromospheric fibrils: Basic properties and MHD kink waves
- An overall view of temperature oscillations in the solar chromosphere with ALMA
- Propagation of Waves above a Plage as Observed by IRIS and SDO
- A novel approach to identify resonant MHD wave modes in solar pores and sunspot umbrae: analysis
- Transverse motions in sunspot super-penumbral fibrils
- Magnetohydrodynamic wave mode identification in circular and elliptical sunspot umbrae: evidence for high order modes
- ALMA observations of the variability of the quiet Sun at millimeter wavelengths
- Small-scale solar jet formation and their associated waves and instabilities
- Tomography of a solar plage with the Tenerife Inversion Code
- Spectropolarimetric Fluctuations in a Sunspot Chromosphere
- Spectroscopic evidence of Alfvén wave damping in the off-limb solar corona
- On the Origin of Magnetic Pertubations associated with the FIP effect
- High-resolution wave dynamics in the lower solar atmosphere
- Laboratory evidence for asymmetric accretion structure upon slanted matter impact in young stars
- Finding the mechanism of wave energy flux damping in solar pores using numerical simulations
- IBIS-A: The IBIS data Archive. High resolution observations of the solar photosphere and chromosphere with contextual data
- High-frequency oscillations in small chromospheric bright features observed with ALMA
- Damping of slow surface kink modes in solar photospheric waveguides modeled by one-dimensional inhomogeneities
- Sausage, kink, and fluting MHD wave modes identified in solar magnetic pores by Solar Orbiter/PHI
- IRIS observations of chromospheric heating by acoustic waves in solar quiet and active regions
- The effect of flow on resonant absorption of slow MHD waves in magnetic flux tubes
- Peculiarity of the oscillation stratification in sunspot penumbrae
- Fast magnetic wave could heat the solar low-beta chromosphere
- Ambipolar Diffusion in the Lower Solar Atmosphere: MHD Simulations of a Sunspot
- Dominance of 2-Minute Oscillations near the Alfvén Surface
- Unveiling the True Nature of Plasma Dynamics from the Reference Frame of a Super-penumbral Fibril
- Propagation of transverse waves in the solar chromosphere probed at different heights with ALMA sub-bands
- Magneto-acoustic oscillations observed in a solar plage region
- On the formation height of low-corona and chromospheric channels of the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO)
- Wave Conversion, Decay and Heating in a Partially Ionized Two-Fluid Magneto-Atmosphere
- Observation of solar coronal heating powered by magneto-acoustic oscillations in a moss region
- Spectropolarimetric investigation of magnetohydrodynamic wave modes in the photosphere: First results from PHI on board Solar Orbiter
- Spectroscopic study of solar transition region oscillations in the quiet-Sun observed by IRIS using Si IV spectral line
- Coronal Abundance Fractionation Linked to Chromospheric Transverse MHD Waves in a Solar Active Region Observed with FISS/GST and EIS/Hinode
- Oblique Quasi-Kink Modes in Solar Coronal Slabs Embedded in an Asymmetric Magnetic Environment: Resonant Damping, Phase and Group Diagrams
- Comparison of exact and approximate MHD slow body mode solutions in photospheric waveguides
- Chromosphere of the quiet sun -- I. Shock and current-sheet dynamics and heating
- Power distribution of oscillations in the atmosphere of a plage region: Joint observations with ALMA, IRIS and SDO
- Transverse vertical oscillations during the contraction and expansion of coronal loops
- Modeling of Chromospheric Features and Dynamics in Solar Plage
- Transverse waves in coronal flux tubes with thick boundaries: The effect of longitudinal flows
- A Search for High-Frequency Coronal Brightness Variations in the 21 August 2017 Total Solar Eclipse
- The Sun at millimeter wavelengths IV. Magnetohydrodynamic waves in small-scale bright features
- Onset of 2D magnetic reconnection in the solar photosphere, chromosphere and corona
- Transverse oscillations in 3D along Ca II K bright fibrils in the solar chromosphere
- Behaviour of oscillations in loop structures above active regions
- ALMA Observations of Solar Spicules in a Polar Coronal Hole
- Modeling the effects of a lightbridge on oscillations in a solar pore
- Understanding the magnetic field and plasma- along umbral fan loops traced using 3-min slow waves
- Alfvén wave propagation, reflection and trapping in the solar wind
- Concurrent Kink and Sausage Waves in A Crescent Shaped Structure Over A Limb Prominence
- Multi-height Identification of Sausage and Fluting Eigenmodes in a Solar Pore
- Chromospheric Heating by Acoustic Waves Compared to Radiative Cooling: II -- Revised Grid of Models
- Effects of background periodic flow on MHD fast wave propagation to a coronal loop
- The Sun at millimeter wavelengths V. Magnetohydrodynamic waves in a fibrillar structure