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The top documents tagged [x10 flare]
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x10 flare
Flare energy and fast electrons via Alfvén waves H. S. Hudson & L. Fletcher SSL/Berkeley and Glasgow U. Predictions for Hinode/SOT flare observations.
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Xu et al., ApJ 607, L131, 2004: or, how do flare footpoints work? First flare observations in the infrared 1.56 nominally is as deep as deep can be (the.
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The Change of Magnetic Inclination Angles Associated with Flares Yixuan Li April 1,2008.
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Contraction of flaring loops — the evidence of magnetic reconnection in sheared core fields Haisheng Ji Purple Mountain Observatory Nanjing, 210008, China.
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Http://gong.nso.eduRudi Komm 1 GONG & STEREO What is this helioseismologist doing here?? – “We all study phenomena that are driven or strongly influenced.
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Relaxation of Sheared Magnetic fields — a Process of Contraction
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