Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed In Active Region NOAA 11167
arXiv:1912.11792 · doi:10.3847/1538-4357/ab655f
Abstract
We report a detailed observational study of two quasi-periodic fast-propagating (QFP) magnetosonic wave events occurred on 2011 March 09 and 10, respectively. Interestingly, both the two events have two wave trains (WTs): one main and strong (WT-1) whereas the second appears small and weak (WT-2). Peculiar and common characteristics of the two events are observed, namely: 1) the two QFP waves are accompanied with brightenings during the whole stage of the eruptions; 2) both the two main wave trains are nearly propagating along the same direction; 3) EUV waves are found to be associated with the two events. Investigating various aspects of the target events, we argue that: 1) the second event is accompanied with a flux rope eruption during the whole stage; 2) the second event eruption produces a new filament-like (FL) dark feature; 3) the ripples of the two WT-2 QFP waves seem to result from different triggering mechanisms. Based on the obtained observational results, we propose that the funnel-like coronal loop system is indeed playing an important role in the two WT-1 QFP waves. The development of the second WT-2 QFP wave can be explained as due to the dispersion of the main EUV front. The co-existence of the two events offer thereby a significant opportunity to reveal what driving mechanisms and structures are tightly related to the waves.
arXiv comment9 figures,ApJ,accepted, December 19,2019
References in corpus (46)
- Observation of An Evolving Magnetic Flux Rope Prior To and During A Solar Eruption
- 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
- Observations of Turbulent Magnetic Reconnection Within a Solar Current Sheet
- Direct Imaging by SDO AIA of Quasi-periodic Fast Propagating Waves of ~2000 km/s in the Low Solar Corona
- The Driver of Coronal Mass Ejections in the Low Corona: A Flux Rope
- First SDO AIA Observations of a Global Coronal EUV "Wave": Multiple Components and "Ripples"
- First Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations
- 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
- On a solar blowout jet: driven mechanism and the formation of cool and hot components
- Observational Study Of the Quasi-Periodic Fast Propagating Magnetosonic Waves and the Associated Flare on 2011 May 30
- SOHO/SUMER Observations of Prominence Oscillation Before Eruption
- SDO/AIA Observations of Large-Amplitude Longitudinal Oscillations in a Solar Filament
- SDO/AIA Observations of Secondary Waves Generated by Interaction of the 2011 June 7 Global EUV Wave With Solar Coronal Structures
- The Relation between EIT Waves and Coronal Mass Ejections
- Simultaneous Observations of a Large-Scale Wave Event in the Solar Atmosphere: From Photosphere to Corona
- Diffraction, Refraction, and Reflection of An Extreme-Ultraviolet Wave Observed during Its Interactions with Remote Active Regions
- Three-dimensional MHD Simulations of Solar Prominence Oscillations in a Magnetic Flux Rope
- Observations of a Quasi-Periodic Fast Propagating Magnetosonic Wave in Multi-Wavelength and Its Interaction with Other Magnetic Structures
- A quasi-periodic fast-propagating magnetosonic wave associated with the eruption of a magnetic flux rope
- 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
- On a small-scale EUV wave: the driving mechanism and the associated oscillating filament
- Pre-Eruptive Magnetic Reconnection within a Multi-Flux-Rope System in the Solar Corona
- Solar Magnetic Flux Ropes
- Forward Modelling of Standing Kink Modes in Coronal Loops II. Applications
- Quasi-Periodic Radio Bursts Associated with Fast-mode Waves near a Magnetic Null Point
- Forward Modelling of Standing Slow Modes in Flaring Coronal Loops
- First Unambiguous Imaging of Large-Scale Quasi-Periodic Extreme-Ultraviolet Wave or Shock
- Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling
- EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
- Forward Modelling of Standing Kink Modes in Coronal Loops I. Synthetic Views
- SDO/AIA and Hinode/EIS Observations of Interaction Between an EUV Wave and Active Region Loops
- Flux Rope Breaking and Formation of a Rotating Blowout Jet
- A Quasi-periodic propagating wave and EUV waves excited simultaneously in a solar eruption event
- Global Coronal Waves
- Observation of quasi-periodic solar radio bursts associated with propagating fast-mode waves
- 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
- Impacts of EUV Wavefronts on Coronal Structures in Homologous Coronal Mass Ejections
- Stochastic transients as a source of quasi-periodic processes in the solar atmosphere
- Fast magnetoacoustic waves in a fan structure above the coronal magnetic null point
- Coronal Density and Temperature Profiles Calculated by Forward Modeling EUV Emission Observed by SDO/AIA
- Secondary fast magnetoacoustic waves trapped in randomly structured plasmas
Cited by in corpus (6)
- Coronal Quasi-periodic Fast-mode Propagating Wave Trains
- Diagnosing a Solar Flaring Core with Bidirectional Quasi-Periodic Fast Propagating Magnetoacoustic Waves
- Observations of a Flare-ignited broad Quasi-periodic Fast-propagating wave train
- Light Bridges Can Suppress the Formation of Coronal Loops
- Modeling the Excitation, Propagation and Damping of Quasi-Periodic Fast Magnetosonic Waves in Realistic Coronal Active Region Magnetic Field Structures
- Quasi-Periodic Pulsations Detected in Ly and Nonthermal Emissions During Solar Flares