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- 10:26, 11 February 2013 (diff | hist) Passages of Electron Beams
- 10:22, 11 February 2013 (diff | hist) Passages of Electron Beams
- 10:20, 11 February 2013 (diff | hist) Passages of Electron Beams
- 10:08, 11 February 2013 (diff | hist) Passages of Electron Beams
- 15:50, 27 January 2013 (diff | hist) N Passages of Electron Beams (Created page with "== Introduction== Solar flares involve production of energetic electron beams. They carry a significant amount of magnetic energy released and therefore play a key role in flare...")
- 15:47, 27 January 2013 (diff | hist) Tracing Electron Beams with Radio Dynamic Imaging Spectroscopy (top)
- 22:32, 26 January 2013 (diff | hist) N Tracing Electron Beams with Radio Dynamic Imaging Spectroscopy (Passages of fast electron beams in the low corona are traced through radio observations.)
- 21:29, 26 January 2013 (diff | hist) N File:193f3.jpg (Type IIIdm burst centroids as a function of frequency (colored from blue to red for increasing frequencies), showing trajectories of fast electron beams in the solar corona.) (top)
- 21:17, 26 January 2013 (diff | hist) File:193f2.jpg (top)
- 21:15, 26 January 2013 (diff | hist) N File:193f2.jpg ((A) Composite image of AR 11339 from SDO/AIA on 2011 November 5. (B) GOES SXR flux showing the M1.8 flare and its aftermath. The coronal jet occurred between 21:18-21:25 UT (dashed vertical lines). (C-D) VLA dynamic spectra in which type IIIdm bursts (the)
- 21:14, 26 January 2013 (diff | hist) N File:193f1 VLA.jpg (The Karl G. Jansky Very Large Array, located on the Plains of San Agustin, about 80 km west of Socorro, New Mexico, USA (Photo by Bin Chen).) (top)