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Understanding the Physical Nature of Coronal "EIT Waves" (CROSBI ID 234802)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Long, David M. ; Bloomfield, D. Shaun ; Chen, P. F. ; Downs, Cooper ; Gallagher, Peter T. ; Kwon, Ryun Young ; Vanninathan, Kamalam ; Veronig, Astrid M. ; Vourlidas, Angelos ; Vršnak, Bojan et al. Understanding the Physical Nature of Coronal "EIT Waves" // Solar physics, 292 (2017), 1; UNSP 7-1-UNSP 7-31. doi: 10.1007/s11207-016-1030-y

Podaci o odgovornosti

Long, David M. ; Bloomfield, D. Shaun ; Chen, P. F. ; Downs, Cooper ; Gallagher, Peter T. ; Kwon, Ryun Young ; Vanninathan, Kamalam ; Veronig, Astrid M. ; Vourlidas, Angelos ; Vršnak, Bojan ; Warmuth, Alexander ; Žic, Tomislav

engleski

Understanding the Physical Nature of Coronal "EIT Waves"

For almost 20 years the physical nature of globally propagating waves in the solar corona (commonly called "EIT waves"') has been controversial and subject to debate. Additional theories have been proposed over the years to explain observations that did not agree with the originally proposed fast-mode wave interpretation. However, the incompatibility of observations made using the Extreme-ultraviolet Imaging Telescope (EIT) onboard the Solar and Heliospheric Observatory with the fast-mode wave interpretation was challenged by differing viewpoints from the twin Solar Terrestrial Relations Observatory spacecraft and data with higher spatial and temporal resolution from the Solar Dynamics Observatory. In this article, we reexamine the theories proposed to explain EIT waves to identify measurable properties and behaviours that can be compared to current and future observations. Most of us conclude that the so-called EIT waves are best described as fast-mode large-amplitude waves or shocks that are initially driven by the impulsive expansion of an erupting coronal mass ejection in the low corona.

Coronal mass ejections ; low coronal signatures ; Waves ; magnetohydrodynamic ; Waves ; propagation ; Waves ; shock

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Podaci o izdanju

292 (1)

2017.

UNSP 7-1-UNSP 7-31

objavljeno

0038-0938

10.1007/s11207-016-1030-y

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Fizika

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