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Combined display of all available logs of RHESSI Wiki. You can narrow down the view by selecting a log type, the user name (case-sensitive), or the affected page (also case-sensitive).- 06:21, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:All fov distribs ff.png" (Distributions of upward (blue solid) and downward (red dashed) Poynting flux values in plage-like pixels in AR 10930. Upward wins! )
- 06:20, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:All fov plage mask.png" (Mask of plage-like fields in AR 10930, i.e., pixels for which the vector magnetic field was estimated and filling-factor-weighted |Bz| was between 100 and 1500 Mx cm−2 and inclinations were less than 30 from the vertical.)
- 06:15, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:Joint poynt map.png" (Splice of Lp_hr_vectors_ff_4.png and Lp_poynting_ff_4.png )
- 06:03, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:Lp poynting ff 4.png" (Map of Poynting flux, from FLCT velocities, from http://arxiv.org/abs/1402.4794 )
- 05:56, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:Lp hr vectors ff 4.png" (Vector magnetogram from SP and overlain velocities inferred by LCT, from http://arxiv.org/abs/1402.4794)
- 04:40, 20 September 2014 BrianWelsch (Talk | contribs) uploaded "File:Parker winding nanoflares.png" (Parker's cartoon of footpoint motions leading to braiding of coronal magnetic fields. From "Magnetic Neutral Sheets in Evolving Fields - Part Two - Formation of the Solar Corona," by E.N. Parker, Astrophysical Journal, Vol.264, P. 642, 1983. ADS link: ht)