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 - Regions Field - Document - PDFSEARCH.IO

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	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 Document Date: 2014-03-25 12:36:54 Open Document File Size: 108,88 KB Share Result on Facebook Event Natural Disaster / / Technology X-ray / / SocialTag Space plasmas Astrophysics Light sources Sun Magnetic reconnection Coronal mass ejection Solar flare Corona Magnetic field Physics

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 eruptionAdd to Reading List