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Showing 1 to 2 of 2 for “"Sun; flares"”.
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Evolution of 3-d magnetic topology in flare-productive active regions
Solar eruptive phenomena, such as flares and coronal mass ejections (CMEs), derive their energy from complex magnetic fields and are the principal source of disturbances that affect space weather. Although physical mechanism and dynamic morphology of flares have been a subject of intense research, …
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Dynamics of filaments, flares and coronal mass ejections (CMEs)
… surface phenomena such as filament eruptions, flares, the coronal mass ejections (CMEs), the core of so-called solar activity, and the properties of the associated magnetic field for the development of forecasts of solar activity and space weather. Both statistical and case studies have been …