User contributions for Hhudson

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20:0420:04, 19 October 2026 diff hist +6,216‎ N ALEXIS: When and Where is that Flare ‎ Created page with "{{Infobox Nugget |name = Nugget |title = Alexis: When and Where is that Flare? |number = 538 |first_author = Jorge R. PADIAL DOBLE |second_author = Kelly HOLLEY-BOCKELMANN |publish_date = October 26, 2026 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::537}} }} == A light curve without a location == Every X5.0 solar flare headline you have read about is named after a single number: the soft X-ray flux of the entire unresolved..." current
19:5419:54, 19 October 2026 diff hist +2‎ Alexis: When and Where is that Flare? ‎No edit summary current
11:1211:12, 19 October 2026 diff hist +1‎ Alexis: When and Where is that Flare? ‎No edit summary
11:1011:10, 19 October 2026 diff hist 0‎ N File:538 f1.png ‎No edit summary current
11:1011:10, 19 October 2026 diff hist +6,211‎ N Alexis: When and Where is that Flare? ‎ Created page with "{{Infobox Nugget |name = Nugget |title = Alexis: When and Where is that Flare? |number = 538 |first_author = Jorge R. PADIAL DOBLE |second_author = Kelly HOLLEY-BOCKELMANN |publish_date = October 26, 2026 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::537}} }} == A light curve without a location == Every X5.0 solar flare headline you have read about is named after a single number: the soft X-ray flux of the entire unresolved..."

08:5708:57, 11 October 2026 diff hist +13‎ The Hale Sector Boundary links flares to global magnetic fields ‎ →‎Introduction current

09:2909:29, 10 October 2026 diff hist +4‎ SolarNuggets ‎No edit summary current
09:2809:28, 10 October 2026 diff hist +314‎ SolarNuggets ‎No edit summary
09:2509:25, 10 October 2026 diff hist 0‎ N File:Icon537.png ‎No edit summary current
08:4508:45, 10 October 2026 diff hist +34‎ The Hale Sector Boundary links flares to global magnetic fields ‎ →‎Conclusions
08:4308:43, 10 October 2026 diff hist +1‎ The Hale Sector Boundary links flares to global magnetic fields ‎ →‎Introduction
08:4208:42, 10 October 2026 diff hist +241‎ The Hale Sector Boundary links flares to global magnetic fields ‎No edit summary
08:3908:39, 10 October 2026 diff hist 0‎ File:537f1.png ‎ Hhudson uploaded a new version of File:537f1.png current

19:5319:53, 9 October 2026 diff hist +124‎ The Hale Sector Boundary links flares to global magnetic fields ‎ →‎Conclusions
19:4919:49, 9 October 2026 diff hist 0‎ The Hale Sector Boundary links flares to global magnetic fields ‎No edit summary
19:4219:42, 9 October 2026 diff hist 0‎ The Hale Sector Boundary links flares to global magnetic fields ‎ →‎References
19:4119:41, 9 October 2026 diff hist +1‎ The Hale Sector Boundary links flares to global magnetic fields ‎No edit summary
19:3919:39, 9 October 2026 diff hist +3,600‎ N The Hale Sector Boundary links flares to global magnetic fields ‎ No. 537 initial upload
19:2319:23, 9 October 2026 diff hist 0‎ N File:537f2..png ‎No edit summary current
19:2219:22, 9 October 2026 diff hist 0‎ N File:537f1.png ‎No edit summary

20:1620:16, 2 October 2026 diff hist +96‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ →‎EVE power spectra current

20:2120:21, 29 September 2026 diff hist 0‎ SolarNuggets ‎No edit summary

13:5513:55, 28 September 2026 diff hist +339‎ SolarNuggets ‎ Added No. 536
13:5013:50, 28 September 2026 diff hist 0‎ N File:Icon536.png ‎No edit summary current
07:3407:34, 28 September 2026 diff hist +64‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ →‎EVE power spectra
07:3107:31, 28 September 2026 diff hist −1‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ →‎What do power spectra show us?
07:2507:25, 28 September 2026 diff hist +26‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎No edit summary

10:0610:06, 27 September 2026 diff hist +24‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ →‎Conclusions
10:0310:03, 27 September 2026 diff hist +77‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ →‎EVE power spectra
10:0010:00, 27 September 2026 diff hist 0‎ N File:536f2.png ‎No edit summary current
10:0010:00, 27 September 2026 diff hist 0‎ N File:536f1.png ‎No edit summary current
09:5909:59, 27 September 2026 diff hist +237‎ Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎No edit summary
09:5609:56, 27 September 2026 diff hist +5,826‎ N Photospheric flows in Sun-as-a-star EUV Doppler spectra ‎ No. 536 without figures

20:3920:39, 17 September 2026 diff hist +274‎ SolarNuggets ‎ Added No. 535
20:3520:35, 17 September 2026 diff hist 0‎ N File:Icon535.png ‎No edit summary current
20:3320:33, 17 September 2026 diff hist +36‎ Why do only some fast CMEs produce sustained gamma-ray emissions? ‎ author's fixes current

16:4916:49, 16 September 2026 diff hist −2‎ Why do only some fast CMEs produce sustained gamma-ray emissions? ‎ →‎Conclusions
16:3216:32, 16 September 2026 diff hist 0‎ N File:535f3.png ‎No edit summary current
16:3116:31, 16 September 2026 diff hist 0‎ Why do only some fast CMEs produce sustained gamma-ray emissions? ‎No edit summary
16:3016:30, 16 September 2026 diff hist 0‎ N File:535f1.png ‎No edit summary current
16:2816:28, 16 September 2026 diff hist 0‎ N File:535f2.png ‎No edit summary current
16:2416:24, 16 September 2026 diff hist +4,837‎ N Why do only some fast CMEs produce sustained gamma-ray emissions? ‎ Created page with "{{Infobox Nugget |name = Nugget |title = Why do only some fast CMEs produce sustained gamma-ray emissions? |number = 535 |first_author = Ratul MOHAN |publish_date = September 14, 2026 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::534}} }} == Introduction == Certain strong solar flares may accelerate particles producing intense gamma-ray emissions during their impulsive phase. In some flares, however, gamma rays with energies >..."

14:0514:05, 4 September 2026 diff hist +17‎ A New Route to Coronal Vector Magnetometry ‎ author's fixes current
08:3508:35, 4 September 2026 diff hist 0‎ SolarNuggets ‎No edit summary
08:3408:34, 4 September 2026 diff hist +254‎ SolarNuggets ‎ Added No. 534
08:3008:30, 4 September 2026 diff hist 0‎ N File:Icon534.png ‎No edit summary current
08:2708:27, 4 September 2026 diff hist +7‎ A New Route to Coronal Vector Magnetometry ‎ →‎Conclusion
08:2608:26, 4 September 2026 diff hist +2‎ A New Route to Coronal Vector Magnetometry ‎ →‎Getting at the Stokes parameters
07:4907:49, 4 September 2026 diff hist +31‎ A New Route to Coronal Vector Magnetometry ‎ →‎Introduction
07:4707:47, 4 September 2026 diff hist +59‎ A New Route to Coronal Vector Magnetometry ‎No edit summary

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