Homologous large-amplitude Nonlinear fast-mode Magnetosonic Waves Driven by Recurrent Coronal Jets
arXiv:1805.12303 · doi:10.3847/1538-4357/aac9be
Abstract
The detailed observational analysis of a homologous Extreme-ultraviolet (EUV) wave event is presented to study the driving mechanism and the physical property of the EUV waves, combining high resolution data taken by the Solar Dynamics Observatory and the Solar TErrestrial RElations Observatory. It is observed that four homologous EUV waves originated from the same active region AR11476 within about one hour, and the time separations between consecutive waves were of 8 - 20 minutes. The waves showed narrow arc-shaped wavefronts and propagated in the same direction along a large-scale transequatorial loop system at a speed of 648 - 712 km/s and a deceleration of 0.985 - 1.219 km/s2. The EUV waves were accompanied by weak flares, coronal jets, and radio type III bursts, in which the EUV waves were delayed with respect to the start times of the radio type III bursts and coronal jets about 2 - 13 and 4 - 9 minutes, respectively. Different to previous studies of homologous EUV waves, no coronal mass ejections were found in the present event. Based on the observational results and the close temporal the spatial relationship between the EUV waves and the coronal jets, for the first time, we propose that the observed homologous EUV waves were large-amplitude nonlinear fast-mode magnetosonic waves or shocks driven by the associated recurrent coronal jets, resemble the generation mechanism of a piston shock in a tube. In addition, it is found that the recurrent jets were tightly associated with the alternating flux cancellation and emergence in the eruption source region and radio type III bursts.
arXiv comment21 pages, 6 figures, 2 tables. Accepted by ApJ
References in corpus (69)
- Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
- Solar Coronal Jets: Observations, Theory, and Modeling
- The Interaction of Successive Coronal Mass Ejections: A Review
- Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)
- On a Coronal Blowout Jet: The First Observation of a Simultaneously Produced Bubble-like CME and a Jet-like CME in a Solar Event
- Quasi-periodic Fast-mode Wave Trains Within a Global EUV Wave and Sequential Transverse Oscillations Detected by SDO/AIA
- Circular Ribbon Flares and Homologous Jets
- Observations and Interpretation of a Low Coronal Shock Wave Observed in the EUV by the SDO/AIA
- Sympathetic Partial and Full Filament Eruptions Observed in One Solar Breakout Event
- The Kinematics of a Globally Propagating Disturbance in the Solar Corona
- 'EUV Waves' are Waves: First Quadrature Observations of an EUV Wave from STEREO
- On Sun-to-Earth Propagation of Coronal Mass Ejections
- Direct Imaging by SDO AIA of Quasi-periodic Fast Propagating Waves of ~2000 km/s in the Low Solar Corona
- Kinematics and Fine Structure of An Unwinding Polar Jet Observed by SDO/AIA
- Large-scale Coronal Propagating Fronts in Solar Eruptions as Observed by the Atmospheric Imaging Assembly on Board the Solar Dynamics Observatory\,--\,An Ensemble Study
- Large-scale Bright Fronts in the Solar Corona: A Review of "EIT waves"
- Homologous Helical Jets: Observations by IRIS, SDO and Hinode and Magnetic Modeling with Data-Driven Simulations
- Investigation of the Formation and Separation of An EUV Wave from the Expansion of A Coronal Mass Ejection
- Successive X-class flares and coronal mass ejections driven by shearing motion and sunspot rotation in active region NOAA 12673
- STEREO quadrature observations of the 3D structure and driver of a global coronal wave
- A Chain of Winking (Oscillating) Filaments Triggered by an Invisible Extreme-Ultraviolet Wave
- Numerical Experiments of Wave-Like Phenomena Caused by the Disruption of an Unstable Magnetic Configuration
- What is the Nature of EUV Waves? First STEREO 3D Observations and Comparison with Theoretical Models
- Simultaneous Transverse Oscillations of a Prominence and a Filament and Longitudinal Oscillation of another Filament Induced by a Single Shock Wave
- On a solar blowout jet: driven mechanism and the formation of cool and hot components
- Understanding the Physical Nature of Coronal "EIT Waves"
- Toward understanding the early stages of an impulsively accelerated coronal mass ejection
- 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
- Observational Study Of the Quasi-Periodic Fast Propagating Magnetosonic Waves and the Associated Flare on 2011 May 30
- 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
- A Time Series of Filament Eruptions Observed by Three Eyes from Space: From Failed to Successful Eruptions
- Simultaneous Observations of a Large-Scale Wave Event in the Solar Atmosphere: From Photosphere to Corona
- Kinematics of an untwisting solar jet in polar coronal hole observed by SDO/AIA
- Diffraction, Refraction, and Reflection of An Extreme-Ultraviolet Wave Observed during Its Interactions with Remote Active Regions
- Observations of a Quasi-Periodic Fast Propagating Magnetosonic Wave in Multi-Wavelength and Its Interaction with Other Magnetic Structures
- Homologous Jet-Driven Coronal Mass Ejections From Solar Active Region 12192
- Measuring the magnetic field of a trans-equatorial loop system using coronal seismology
- A quasi-periodic fast-propagating magnetosonic wave associated with the eruption of a magnetic flux rope
- Statistical Analysis of Large-scale EUV Waves Observed by STEREO/EUVI
- Simultaneous transverse and longitudinal oscillations in a quiescent prominence triggered by a coronal jet
- On a small-scale EUV wave: the driving mechanism and the associated oscillating filament
- Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause
- A Type II Radio Burst without a Coronal Mass Ejection
- Deceleration and Dispersion of Large-scale Coronal Bright Fronts
- On the Magnetic and Energy Characteristics of Recurrent Homologous Jets from An Emerging Flux
- EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
- SDO/AIA and Hinode/EIS Observations of Interaction Between an EUV Wave and Active Region Loops
- Successive Two-sided loop Jets Caused by Magnetic Reconnection between Two adjacent Filamentary Threads
- Can a Fast-mode EUV Wave Generate a Stationary Front?
- Observations of multiple blobs in homologous solar coronal jets in closed loops
- Sympathetic Solar Filament Eruptions on 2015 March 15
- Magnetic Field Restructuring Associated with Two Successive Solar Eruptions
- Case Study of Four Homologous Large-Scale Coronal Waves Observed on 2010 April 28 and 29
- Successive Homologous Coronal Mass Ejections driven by shearing and converging motions in solar active region NOAA 12371
- Observations of EUV and Soft X-ray Recurring Jets in an Active Region
- Eruption of a plasma blob, associated M-class flare, and large-scale EUV wave observed by SDO
- Homologous white light solar flares driven by photosperic shear motions
- The Association of Solar Flares with Coronal Mass Ejections During the Extended Solar Minimum
- Vertical oscillation of a coronal cavity triggered by an EUV wave
- Simultaneous longitudinal and transverse oscillation in an active filament
- A Statistical Analysis of the Solar Phenomena Associated with Global EUV Waves
- Formation of Coronal Shock Waves
- Mode-Conversion of a Solar Extreme-Ultraviolet Wave over a Coronal Cavity
- Waiting Times of Quasi-homologous Coronal Mass Ejections from Super Active Regions
- Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped Flare
- The surge-like eruption of a miniature filament
- Dispersively Formed Quasi-Periodic Fast Magnetosonic Wavefronts Due to the Eruption of a Nearby Mini-filament
- Coronal and Chromospheric Signatures of Large-Scale Disturbances Associated with a Major Solar Eruption
Cited by in corpus (26)
- Observation and Modeling of Solar Jets
- Stereoscopic Observations of an Erupting Mini-filament Driven Two-Sided-Loop Jet and the Applications for Diagnosing Filament Magnetic field
- Round-trip Slipping Motion of the Circular Flare Ribbon Evidenced in a Fan-spine Jet
- First Unambiguous Imaging of Large-Scale Quasi-Periodic Extreme-Ultraviolet Wave or Shock
- Coronal microjets in quiet-Sun regions observed with the Extreme Ultraviolet Imager onboard Solar Orbiter
- Coronal EUV, QFP, and kink waves simultaneously launched during the course of jet-loop interaction
- Homologous Accelerated Electron Beams, Quasi-periodic fast-propagating Wave and CME Observed in one Fan-spine Jet
- CME-Driven and Flare-Ignited Fast Magnetosonic Waves Successively Detected in a Solar Eruption
- Possible Generation Mechanism for Compressional Alfvénic Spikes as Observed by Parker Solar Probe
- The Birth of a Jet-driven Twin CME and Its Deflection from Remote Magnetic Fields
- Spectroscopic and Stereoscopic Observations of the Solar Jets
- Sympathetic Standard and Blowout Coronal Jets Observed in a Polar Coronal Hole
- Observations of a Flare-ignited broad Quasi-periodic Fast-propagating wave train
- Stereoscopic diagnosing of a filament-cavity flux rope system by tracing the path of a two-sided-loop jet
- A small-scale filament eruption inducing Moreton Wave, EUV Wave and Coronal Mass Ejection
- A new small satellite sunspot triggering recurrent standard- and blowout-coronal jets
- Twin CME Launched by a Blowout Jet Originated from the Eruption of a Quiet-Sun Mini-filament
- Cross-loop propagation of a quasi-periodic extreme-ultraviolet wave train triggered by successive stretching of magnetic field structures during a solar eruption
- The initial morphologies of the wavefronts of extreme ultraviolet waves
- An Extreme Ultraviolet Wave Associated with A Solar Filament Activation
- Recurrent narrow quasi-periodic fast-propagating wave trains excited by the intermittent energy release in the accompanying solar flare
- Birth places of extreme ultraviolet waves driven by impingement of solar jets upon coronal loops
- High-Resolution Observations of a Small-Scale Cancellation Nanoflare: Supporting Evidence for the Cancellation Nanoflare Model
- Decimetric type U solar radio bursts and associated EUV phenomena on 2011 February 9
- Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO
- Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption