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• W2168748223 startingPage "A120" @default.
• W2168748223 abstract "Context. Coronal mass ejections (CMEs) are the most violent phenomena observed on the Sun. Currently, extreme ultraviolet (EUV) images from the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) are providing new insights into the early phase of CME evolution. In particular, observations now show the ejection of magnetic flux ropes from the solar corona and how they evolve into CMEs. While this is the case, these observations are difficult to interpret in terms of basic physical mechanisms and quantities. To fully understand CMEs we need to compare equivalent quantities derived from both observations and theoretical models. This will aid in bridging the gap between observations and models." @default.
• W2168748223 created "2016-06-24" @default.
• W2168748223 creator A5004751935 @default.
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• W2168748223 date "2014-08-01" @default.
• W2168748223 modified "2023-10-16" @default.
• W2168748223 title "Simulating AIA observations of a flux rope ejection" @default.
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• W2168748223 doi "https://doi.org/10.1051/0004-6361/201424019" @default.
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