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- 13:26, 13 April 2026 Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Nonradial to Radial Propagation (hist | edit) [5,435 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Nonradial to Radial Propagation |number = 522 |first_author = Huidong HU |publish_date = April 13, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::521}} }} == Introduction == Solar coronal mass ejections [https://en.wikipedia.org/wiki/Coronal_mass_ejection (CMEs)] are large-scale expulsions of p...")
- 16:27, 11 April 2026 Can EUV Power-Spectral Indices Reveal Imminent Solar Flares? (hist | edit) [7,041 bytes] Hhudson (talk | contribs) (No. 521 initial entry)
- 13:55, 22 March 2026 How energetic can solar flares become? (hist | edit) [4,623 bytes] Hhudson (talk | contribs) (No)
- 13:03, 19 March 2026 Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Flare Loops (hist | edit) [6,411 bytes] Hhudson (talk | contribs) (No. 519 text)
- 21:35, 10 March 2026 When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps (hist | edit) [5,772 bytes] Hhudson (talk | contribs) (No. 518 initial)
- 16:09, 27 February 2026 Observational Evidence Linking Loop Length and Thermal/Nonthermal Peak Timing in Solar Flares (hist | edit) [5,477 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = Observational Evidence Linking Loop Length and Thermal/Nonthermal Peak Timing in Solar Flares |number = 517 |first_author = Solomon PERRIYIL |publish_date = February 23, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::516}} }} == Introduction == Solar flares rapidly convert stored magnetic energy into particle acceleration and plasma heating. In the collisional thick-target pictur...")
- 17:07, 9 February 2026 A fine-scale bright kernel captured by Hi-C 3 in the post-maximum phase of an M-class solar flare (hist | edit) [6,868 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = A fine-scale bright kernel captured by Hi-C 3 in the post-maximum phase of an M-class solar flare |number = 516 |first_author = Sanjiv TIWARI |publish_date = February 9, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::515}} }} == Introduction == The third successful flight (<i>Hi-C Flare</i>) of the High-Resolution Coronal Imager sounding rocket [https://en.wikipedia.org/wiki/Hig...")
- 20:50, 11 January 2026 On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona (hist | edit) [7,040 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona |number = 515 |first_author = Shanwlee SOW MONDAL et al. |publish_date = January 19, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::514}} }} == Introduction == [https://en.wikipedia.org/wiki/Eugene_Parker Parker]'s [https://en.wikipedia.org/wiki/Nanoflare "nanoflare"] hypothesis (Ref. [1]) sugges...")