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- 07:43, 4 September 2026 A New Route to Coronal Vector Magnetometry (hist | edit) [5,572 bytes] Hhudson (talk | contribs) (No. 534 initial upload)
- 14:57, 3 September 2026 Trading Stokes V for Wave Speeds: A New Route to Vector Coronal Magnetometry (hist | edit) [5,015 bytes] Hhudson (talk | contribs) (Created page with "{{Infobox Nugget |name = Nugget |title = Trading Stokes V for Wave Speeds: A New Route to Vector Coronal Magnetometry |first_author = Alin PARASCHIV |publish_date = September 1, 2026 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::533}} }} == Introduction == The magnetic field of the solar corona remains observationally elusive. At the same time, it is absolutely the most fundamental property defining all coronal activity. One o...")
- 19:31, 21 August 2026 The Variance of Solar X-ray Flux (hist | edit) [3,975 bytes] Hhudson (talk | contribs) (No. 533 initial upload)
- 08:11, 5 August 2026 Electron-Ion equilibration in CME-driven shocks (hist | edit) [5,516 bytes] Hhudson (talk | contribs) (No. 532 initial upload)
- 16:52, 3 August 2026 The Source Surface Height Through the Solar Cycle: A Path to Better Solar Wind Forecasts (hist | edit) [5,881 bytes] Hhudson (talk | contribs) (No. 531 initial upload)
- 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)