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- 08:49, 5 July 2026 Filament Eruptions as seen in the Sun-as-a-star H-alpha Spectrum (hist | edit) [7,981 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = Filament Eruptions as seen in the Sun-as-a-star H-alpha Spectrum |number = 530 |first_author = Junyi ZHANG |second_author = Yijun HOU |publish_date = July 6, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::529}} }} == Introduction == Solar filament/prominence eruptions are among the most energetic phenomena in the solar atmosphere and are major drivers of [space weather]. The...")
- 12:54, 23 June 2026 Particle Pressure and CMEs (hist | edit) [4,882 bytes] Hhudson (talk | contribs) (No. 529 initial)
- 09:11, 23 June 2026 Streamer Blow-out CMEs and Particle Pressure (hist | edit) [5,663 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = Streamer Blow-out CMEs |number = 529 |first_author = Hugh HUDSON |second_author = Ed CLIVER |publish_date = June 22, 2026 |next_nugget = TBD |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::528}} }} == Introduction == We know about solar energetic particles [https://en.wikipedia.org/wiki/Solar_energetic_particles (SEPS)] from many observations from instruments on space probes, and also from ground-based...")
- 20:53, 3 June 2026 White-Light and Lyman-alpha Emissions in Solar Flares: Timing, Timescale, Energy, and Scaling (hist | edit) [5,893 bytes] Hhudson (talk | contribs) (No. 528 initial)
- 18:48, 25 May 2026 Space Weather Impact of Three Solar Flares Observed at Millimeter Wavelengths (hist | edit) [7,990 bytes] Hhudson (talk | contribs) (Initial upload No. 527)
- 18:31, 11 May 2026 X-ray Log Letters (hist | edit) [6,797 bytes] Hhudson (talk | contribs) (Most of No. 526)
- 08:39, 28 April 2026 How Extreme Can Solar Flares Get? A Statistical View (hist | edit) [5,610 bytes] Hhudson (talk | contribs) (tg)
- 19:31, 22 April 2026 Observations of Slow Elemental Abundance Decay in Association to CME (hist | edit) [4,283 bytes] Hhudson (talk | contribs) (No. 524 initial)
- 15:43, 21 April 2026 An Unusual Long-Lived Radio Burst Oscillating in Frequency (hist | edit) [4,605 bytes] Hhudson (talk | contribs) (No. 523 initial upload)
- 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)