Prominence Oscillations activated by an EUV wave
arXiv:2202.13147 · doi:10.1016/j.asr.2022.02.053
Abstract
Prominence oscillations are one of interesting phenomena in the solar atmosphere, which can be utilized to infer the embedded magnetic field magnitude. We present here the transverse oscillations of two different prominences located at the East solar limb on 2011 February 11 using the multi-wavebands data of the Atmospheric Imaging Assembly (AIA) on-board the Solar Dynamics Observatory (SDO) satellite. A prominence eruption was observed towards the east direction with an average speed of ~275 km/s. The eruption is fitted with the combination of a linear and an exponential functions of time. An extreme ultraviolet (EUV) wave event was associated with the prominence eruption. This EUV wave triggered the oscillations of both prominences on the East limb. We computed the period of each prominence using the wavelet analysis method. The oscillation period varies from 14 to 22 min. The magnetic field of the prominences was derived, which ranges from 14 to 20 G.
arXiv comment8 pages, 4 figures
References in corpus (47)
- Physics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling
- Quasi-periodic Fast-mode Wave Trains Within a Global EUV Wave and Sequential Transverse Oscillations Detected by SDO/AIA
- Kink oscillations of coronal loops
- First Simultaneous Observation of H-alpha Moreton Wave, EUV Wave, and Filament/Prominence Oscillations
- Large Amplitude Oscillations in Prominences
- Large Amplitude Longitudinal Oscillations in a Solar Filament
- First Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations
- Initiation and Early Kinematic Evolution of Solar Eruptions
- A Chain of Winking (Oscillating) Filaments Triggered by an Invisible Extreme-Ultraviolet Wave
- An active region filament studied simultaneously in the chromosphere and photosphere: I - Magnetic structure
- Simultaneous Transverse Oscillations of a Prominence and a Filament and Longitudinal Oscillation of another Filament Induced by a Single Shock Wave
- Observation and Simulation of Longitudinal Oscillations of an Active Region Prominence
- Large amplitude oscillatory motion along a solar filament
- On the Magnetic Field Strength of Active Region Filaments
- Some interesting topics provoked by the solar filament research in the past decade
- Evidence for collapsing fields in corona and photosphere during the 15 February 2011 X2.2 flare: SDO AIA and HMI Observations
- Three-dimensional MHD Simulations of Solar Prominence Oscillations in a Magnetic Flux Rope
- Magnetic fields of an active region filament from full Stokes analysis of Si I 1082.7 nm and He I 1083.0 nm
- GONG Catalog of Solar Filament Oscillations Near Solar Maximum
- Multicomponent He I 10830 Å profiles in an active filament
- Simultaneous transverse and longitudinal oscillations in a quiescent prominence triggered by a coronal jet
- First Unambiguous Imaging of Large-Scale Quasi-Periodic Extreme-Ultraviolet Wave or Shock
- Large-Amplitude Longitudinal Oscillations Triggered by the Merging of Two Solar Filaments: Observations and Magnetic Field Analysis
- MHD Seismology of a Coronal Loop System by the First Two Modes of Standing Kink Waves
- Global coronal seismology
- Formation and eruption of a flux rope from the sigmoid active region NOAA 11719 and associated M6.5 flare: A multi-wavelength study
- Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling
- A case-study of multi-temperature coronal jets for emerging flux MHD models
- Can a Fast-mode EUV Wave Generate a Stationary Front?
- Diagnostics of Coronal Magnetic Fields Through the Hanle Effect in UV and IR Lines
- Solar Filament Longitudinal Oscillations along a Magnetic Field Tube with Two Dips
- Peculiar Stationary EUV Wave Fronts in the eruption on 2011 May 11
- Study of Failed CME Core Associated with Asymmetric Filament Eruption
- Contracting and Erupting Components of Sigmoidal Active Regions
- Longitudinal filament oscillations enhanced by two C-class flares
- Vertical oscillation of a coronal cavity triggered by an EUV wave
- Simultaneous longitudinal and transverse oscillation in an active filament
- Numerical simulations of large-amplitude oscillations in flux-rope solar prominences
- Damping Mechanisms of the Solar Filament Longitudinal Oscillations in Weak Magnetic Field
- Large-amplitude prominence oscillations following the impact by a coronal jet
- Simultaneous longitudinal and transverse oscillations in filament threads after a failed eruption
- Horizontal photospheric flows trigger a filament eruption
- An Extreme Ultraviolet Wave Associated with A Solar Filament Activation
- MHD Seismology of a loop-like filament tube by observed kink waves
- Filament Eruption Driving EUV Loop Contraction then Expansion above a Stable Filament
- Inference of Magnetic Field in the Coronal Streamer Invoking Kink Wave Motions generated by Multiple EUV Waves
- Fine Structures of an EUV Wave Event from Multi-Viewpoint Observations
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- Extreme-Ultraviolet Wave and Accompanying Loop Oscillations
- Numerical simulations of prominence oscillations triggered by external perturbations
- Interaction of solar jets with filaments: Triggering of large-amplitude filament oscillations
- Study of the excitation of large amplitude oscillations in a prominence by nearby flares
- Numerical study of solar eruption, extreme-ultraviolet wave propagation, and wave-induced prominence dynamics