Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)
By Wei David Liu, L. Ofman. 2014
188 citations recorded by the source corpus.
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 past 15 years, observations from three generations of space-borne EUV telescopes have shaped our understanding of this phenomenon and at the same time led to controversy about its physical nature. Since its launch in 2010, the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) has observed more than 210 global EUV waves in exquisite detail, thanks to its high spatio–temporal resolution and full-disk, wide-temperature coverage. A combination of statistical analysis of this large sample, more than 30 detailed case studies, and data-driven MHD modeling, has been leading their physical interpretations to a convergence, favoring a bimodal composition of an outer, fast-mode magnetosonic wave component and an inner, non-wave CME component. Adding to this multifaceted picture, AIA has also discovered new EUV wave and wave-like phenomena associated with various eruptions, including quasi-periodic fast propagating (QFP) wave trains, magnetic Kelvin–Helmholtz instabilities (KHI) in the corona and associated nonlinear waves, and a variety of mini-EUV waves. Seismological applications using such waves are now being actively pursued, especially for the global corona. We review such advances in EUV wave research focusing on recent SDO/AIA observations, their seismological applications, related data-analysis techniques, and numerical and analytical models.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/cd9bffa85b0bfad0a22b63d1bd25daf25033c644
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- T. Van Doorsselaere
- Giuseppe Nisticò
- Valery M. Nakariakov
- Petr Jelínek
- D. Kolotkov
- R. Erdélyi
- Tongjiang Wang
- Erwin Verwichte
Citations in the corpus
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “The interaction of the wave fronts with the medium results in several additional fronts, ripples or wave trains being formed (Patsourakos and Vourlidas 2009; Liu and Ofman 2014), see also Sect.”
- Decayless low-amplitude kink oscillations: a common phenomenon in the solar corona? (2015, unknown): “Kink oscillations are interpreted as fast magnetoacoustic waves guided by field-aligned non-uniformities of the fast magnetoacoustic speed (see De Moortel & Nakariakov 2012; Liu & Ofman 2014, for recent comprehensive reviews).”