First SDO AIA Observations of a Global Coronal EUV "Wave": Multiple Components and "Ripples"
arXiv:1201.0815 · doi:10.1088/2041-8205/723/1/L53
Abstract
We present the first SDO AIA observations of a global coronal EUV disturbance (so-called "EIT wave") revealed in unprecedented detail. The disturbance observed on 2010 April 8 exhibits two components: one diffuse pulse superimposed on which are multiple sharp fronts that have slow and fast components. The disturbance originates in front of erupting coronal loops and some sharp fronts undergo accelerations, both effects implying that the disturbance is driven by a CME. The diffuse pulse, propagating at a uniform velocity of 204-238 km/s with very little angular dependence within its extent in the south, maintains its coherence and stable profile for ~30 minutes. Its arrival at increasing distances coincides with the onsets of loop expansions and the slow sharp front. The fast sharp front overtakes the slow front, producing multiple "ripples" and steepening the local pulse, and both fronts propagate independently afterwards. This behavior resembles the nature of real waves. Unexpectedly, the amplitude and FWHM of the diffuse pulse decrease linearly with distance. A hybrid model, combining both wave and non-wave components, can explain many, but not all, of the observations. Discoveries of the two-component fronts and multiple ripples were made possible for the first time thanks to AIA's high cadences (10-20 s) and high signal-to-noise ratio.
7 pages, 5 figures
References in corpus (4)
Cited by in corpus (68)
- Coronal heating by MHD waves
- Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)
- Magnetohydrodynamic Modeling of the Solar Eruption on 2010 April 8
- First Simultaneous Observation of H-alpha Moreton Wave, EUV Wave, and Filament/Prominence Oscillations
- Large-scale Coronal Propagating Fronts in Solar Eruptions as Observed by the Atmospheric Imaging Assembly on Board the Solar Dynamics Observatory\,--\,An Ensemble Study
- On the Nature and Genesis of EUV Waves: A Synthesis of Observations from SOHO, STEREO, SDO, and Hinode
- First Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations
- Investigation of the Formation and Separation of An EUV Wave from the Expansion of A Coronal Mass Ejection
- A Chain of Winking (Oscillating) Filaments Triggered by an Invisible Extreme-Ultraviolet Wave
- Simultaneous Transverse Oscillations of a Prominence and a Filament and Longitudinal Oscillation of another Filament Induced by a Single Shock Wave
- Understanding the Physical Nature of Coronal "EIT Waves"
- Secondary Waves, and/or the "Reflection" From and "Transmission" Through a Coronal Hole of an EUV Wave Associated With the 2011 February 15 X2.2 Flare Observed With SDO/AIA and STEREO/EUVI
- A New Tool for CME Arrival Time Prediction Using Machine Learning Algorithms: CAT-PUMA
- SDO/AIA Observations of Secondary Waves Generated by Interaction of the 2011 June 7 Global EUV Wave With Solar Coronal Structures
- Evidence for the Wave Nature of an Extreme Ultraviolet Wave Observed by the Atmospheric Imaging Assembly Onboard the Solar Dynamics Observatory
- Ubiquitous rotating network magnetic fields and EUV cyclones in the quiet Sun
- Global Numerical Modeling of Energetic Proton Acceleration in a Coronal Mass Ejection Traveling through the Solar Corona
- Diffraction, Refraction, and Reflection of An Extreme-Ultraviolet Wave Observed during Its Interactions with Remote Active Regions
- A Truly Global Extreme Ultraviolet Wave from the SOL2017-09-10 X8.2+ Solar Flare-Coronal Mass Ejection
- Statistical Analysis of Large-scale EUV Waves Observed by STEREO/EUVI
- A quasi-periodic fast-propagating magnetosonic wave associated with the eruption of a magnetic flux rope
- On a small-scale EUV wave: the driving mechanism and the associated oscillating filament
- Coronal Quasi-periodic Fast-mode Propagating Wave Trains
- Plasma diagnostics of an EIT wave observed by Hinode/EIS and SDO/AIA
- The Wave Properties of Coronal Bright Fronts Observed Using SDO/AIA
- First Unambiguous Imaging of Large-Scale Quasi-Periodic Extreme-Ultraviolet Wave or Shock
- Waves in Solar Coronal Loops
- Coronal response to an EUV wave from DEM analysis
- Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling
- Forward Modelling of Standing Kink Modes in Coronal Loops I. Synthetic Views
- EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
- Measuring the Magnetic Field Strength of the Quiet Solar Corona Using "EIT Waves"
- SDO/AIA and Hinode/EIS Observations of Interaction Between an EUV Wave and Active Region Loops
- Three-dimensional Propagation of the Global EUV Wave associated with a solar eruption on 2021 October 28
- A Quasi-periodic propagating wave and EUV waves excited simultaneously in a solar eruption event
- Global Coronal Waves
- Homologous Accelerated Electron Beams, Quasi-periodic fast-propagating Wave and CME Observed in one Fan-spine Jet
- Using ForeCAT Deflections and Rotations to Constrain the Early Evolution of CMEs
- A blowout jet associated with one obvious extreme-ultraviolet wave and one complicated coronal mass ejection event
- Evolution of fast magnetoacoustic pulses in randomly structured coronal plasmas
- Energetic Proton Propagation and Acceleration Simulated for the Bastille Day Event of July 14, 2000
- Quadrature Observations of Wave and Non-Wave Components and Their Decoupling in an Extreme-Ultraviolet Wave Event
- Formation of Coronal Shock Waves
- Mode-Conversion of a Solar Extreme-Ultraviolet Wave over a Coronal Cavity
- Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection
- Prominence Activation by Coronal Fast Mode Shock
- The energetics of a global shock wave in the low solar corona
- Contribution of Velocity Vortices and Fast Shock Reflection and Refraction to the Formation of EUV Waves in Solar Eruptions
- Numerical Simulation of Coronal Waves interacting with Coronal Holes: I. Basic Features
- A small-scale filament eruption inducing Moreton Wave, EUV Wave and Coronal Mass Ejection
- Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed In Active Region NOAA 11167
- Dynamic Processes of the Moreton Wave on 2014 March 29
- Magnetic reconnection between loops accelerated by a nearby filament eruption
- Cross-loop propagation of a quasi-periodic extreme-ultraviolet wave train triggered by successive stretching of magnetic field structures during a solar eruption
- An Extreme Ultraviolet Wave Associated with A Solar Filament Activation
- The initial morphologies of the wavefronts of extreme ultraviolet waves
- Numerical Simulation of Coronal Waves Interacting with Coronal Holes: II. Dependence on Alfvén Speed Inside the Coronal Hole
- The effect of the environment on the P1/P2 period ratio for kink oscillations of coronal loops
- Numerical Simulation of Coronal Waves Interacting with Coronal Holes: III. Dependence on Initial Amplitude of the Incoming Wave
- An extreme ultraviolet wave generating upward secondary waves in a streamer-like solar structure
- Twin extreme ultraviolet waves in the solar corona
- Geometrical properties of the interaction between oblique incoming coronal waves and coronal holes
- Coronal and Chromospheric Signatures of Large-Scale Disturbances Associated with a Major Solar Eruption
- Numerical study of solar eruption, extreme-ultraviolet wave propagation, and wave-induced prominence dynamics
- Quasi-periodic Fast-mode Magnetosonic Wave Trains Within Coronal Waveguides Associated with Flares and CMEs
- The Formation and Early Evolution of a Coronal Mass Ejection and its Associated Shock Wave on 2014 January 8
- Limb Observations of Global Solar Coronal Extreme-ultraviolet Wavefronts: The Inclination, Kinematics, Coupling with the Expanding Coronal Mass Ejections, and Connection with the Coronal Mass Ejection Driven Shocks
- Shock-Cloud Interaction in the Solar Corona