Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection

@article{Francile2016MoretonAE,
  title={Moreton and EUV Waves Associated with an X1.0 Flare and CME Ejection},
  author={C. Francile and F. L{\'o}pez and H. Cremades and C. Mandrini and M. Luoni and D. Long},
  journal={Solar Physics},
  year={2016},
  volume={291},
  pages={3217-3249}
}
A Moreton wave was detected in active region (AR) 12017 on 29 March 2014 with very high cadence with the H-Alpha Solar Telescope for Argentina (HASTA) in association with an X1.0 flare (SOL2014-03-29T17:48). Several other phenomena took place in connection with this event, such as low-coronal waves and a coronal mass ejection (CME). We analyze the association between the Moreton wave and the EUV signatures observed with the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory… Expand
Dynamic Processes of the Moreton Wave on 2014 March 29.
On 2014 March 29, an intense solar flare classified as X1.0 occurred in the active region 12017. Several associated phenomena accompanied this event, among them a fast-filament eruption, large-scaleExpand
A Small-scale Filament Eruption Inducing a Moreton Wave, an EUV Wave, and a Coronal Mass Ejection
With the launch of SDO, many EUV waves were observed during solar eruptions. However, the joint observations of Moreton and EUV waves are still relatively rare. We present an event that a small-scaleExpand
Observations of Two Successive EUV Waves and Their Mode Conversion
In this paper, we present the observations of two successive fast-mode extreme ultraviolet (EUV) wave events observed on 2016 July 23. Both fast-mode waves were observed by the Atmospheric ImagingExpand
Non-gaussian velocity distributions in solar flares from extreme ultraviolet lines: a possible diagnostic of ion acceleration
In a solar flare, a large fraction of the magnetic energy released is converted rapidly to the kinetic energy of non-thermal particles and bulk plasma motion. This will likely result inExpand
Quasi-periodic pulsations in a solar flare with an unusual phase shift
Two kinds of processes could occur during the flare decay phase: processes of energy release or processes of energy relaxation. Quasi-periodic pulsations (QPPs) of the broadband emission are a goodExpand
Synthetic Radio Imaging for Quiescent and CME-flare Scenarios
Radio observations grant access to a wide range of physical processes through different emission mechanisms. These processes range from thermal and quiescent to eruptive phenomena, such as shockExpand
Quantifying the relationship between Moreton-Ramsey waves and "EIT waves" using observations of 4 homologous wave events
Freely-propagating global waves in the solar atmosphere are commonly observed using Extreme UltraViolet passbands (EUV or "EIT waves"), and less regularly in H-alpha (Moreton-Ramsey waves). DespiteExpand
Preface to Topical Issue: Waves in the Solar Corona: From Microphysics to Macrophysics
Wave and oscillatory processes in the plasma of the solar corona attract growing attention in the context of key challenges in solar physics. For several decades, waves have been considered as one ofExpand
An Eruptive Complex Solar Flare and Events in its Aftermath
Abstract We present a study of the M6.6 flare that occurred on 13 February 2011 in AR 11158. The flare was accompanied by a CME and EUV waves. We use multiwavelength observations from the ground:Expand
Are CMEs capable of producing Moreton waves? A case study: the 2006 December 6 event
Fil: Krause, Gustavo Javier. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico Conicet - Cordoba. Instituto de Estudios Avanzados En Ingenieria y Tecnologia.Expand

References

SHOWING 1-10 OF 89 REFERENCES
Observations and interpretation of a low coronal shock wave observed in the EUV by the SDO/AIA
Taking advantage of both the high temporal and spatial resolutions of the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory, we studied a limb coronal shock wave and its associatedExpand
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)
Global extreme-ultraviolet (EUV) waves are spectacular traveling disturbances in the solar corona associated with energetic eruptions such as coronal mass ejections (CMEs) and flares. Over the pastExpand
ON THE ORIGIN OF THE SOLAR MORETON WAVE OF 2006 DECEMBER 6
We analyzed ground- and space-based observations of the eruptive flare (3B/X6.5) and associated Moreton wave (~850 km s–1; ~270° azimuthal span) of 2006 December 6 to determine the wave driver—eitherExpand
ANALYSIS OF A GLOBAL MORETON WAVE OBSERVED ON 2003 OCTOBER 28
We study the well-pronounced Moreton wave that occurred in association with the X17.2 flare/CME event of 2003 October 28. This Moreton wave is striking for its global propagation and two separateExpand
First Simultaneous Observation of an Hα Moreton Wave, EUV Wave, and Filament/Prominence Oscillations
We report on the first simultaneous observation of an Hα Moreton wave, the corresponding EUV fast coronal waves, and a slow and bright EUV wave (typical EIT wave). We observed a Moreton wave,Expand
A multiwavelength study of solar flare waves. I. Observations and basic properties
Propagating wave-like disturbances associated with solar flares - commonly observed in the chromosphere as Moreton waves - have been known for several decades. Recently, the phenomenon has come backExpand
A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation
The study of solar flare waves - globally propagating wave-like disturbances usually observed in Hα as Moreton waves - has recently come back into focus prompted by the observation of coronal wavesExpand
X-Ray Expanding Features Associated with a Moreton Wave
We report on the simultaneous observation of a Moreton wave in Hα and two kinds of coronal expanding features in soft X-rays near the solar limb. We consider the faster X-ray feature and the slowerExpand
SDO/AIA OBSERVATIONS OF SECONDARY WAVES GENERATED BY INTERACTION OF THE 2011 JUNE 7 GLOBAL EUV WAVE WITH SOLAR CORONAL STRUCTURES
We present Solar Dynamics Observatory/Atmospheric Imaging Assembly observations of the interaction of a global EUV wave on 2011 June 7 with active regions (ARs), coronal holes (CHs), and coronalExpand
Synthesis of CME-Associated Moreton and EIT Wave Features from MHD Simulations
Soft X-ray (SXR) waves, EIT waves, and Hα Moreton waves are all associated with coronal mass ejections (CMEs). The knowledge of the characteristics about these waves is crucial for the understandingExpand
...
1
2
3
4
5
...