Solar Sigmoidal Active Regions: From Formation to Eruption The formation, evolution and eruption of solar active regions is a main theme in solar physics. Ultimately the goal is predicting when, where and how an eruption

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Date: 2014-03-25 12:36:54 Space plasmas Astrophysics Light sources Sun Magnetic reconnection Coronal mass ejection Solar flare Corona Magnetic field Physics Plasma physics Astronomy		Solar Sigmoidal Active Regions: From Formation to Eruption The formation, evolution and eruption of solar active regions is a main theme in solar physics. Ultimately the goal is predicting when, where and how an eruption Add to Reading List Source URL: www.mssl.ucl.ac.uk Download Document from Source Website File Size: 108,88 KB Share Document on Facebook

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