User contributions for Hhudson
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30 May 2025
- 13:0613:06, 30 May 2025 diff hist −1 The Sun's open-closed flux boundary and the origin of the slow solar wind No edit summary current
- 13:0413:04, 30 May 2025 diff hist +526 SolarNuggets No edit summary current
- 12:5712:57, 30 May 2025 diff hist 0 N File:Icon496.png No edit summary current
- 12:5712:57, 30 May 2025 diff hist 0 N File:Icon497.png No edit summary current
- 12:4612:46, 30 May 2025 diff hist 0 File:497f2.png Hhudson uploaded a new version of File:497f2.png current
- 12:2112:21, 30 May 2025 diff hist +1 The Sun's open-closed flux boundary and the origin of the slow solar wind →Introduction
- 12:2112:21, 30 May 2025 diff hist +4 The Sun's open-closed flux boundary and the origin of the slow solar wind author's fixes
29 May 2025
- 13:2213:22, 29 May 2025 diff hist +6,219 N The Sun's open-closed flux boundary and the origin of the slow solar wind No. 497 initial upload
- 13:1013:10, 29 May 2025 diff hist 0 N File:497f2.png No edit summary
- 13:1013:10, 29 May 2025 diff hist 0 N File:497f1.png No edit summary current
22 May 2025
- 14:4614:46, 22 May 2025 diff hist −6 Delay of Near-Relativistic Electrons →Observations by Parker Solar Probe/ISIS: author's input current
- 11:4911:49, 22 May 2025 diff hist +6,159 N Delay of Near-Relativistic Electrons Created page with "{{Infobox Nugget |name = Nugget |title = Delay of Near-Relativistic Electrons |number = 496 |first_author = Grant MITCHELL |publish_date = May 19, 2025 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::495}} }} == Introduction == [https://en.wikipedia.org/wiki/Solar_radio_emission Solar radio emission] at long wavelengths (20-1000 MHz) has a very common pattern: type III bursts feature striking drifts from high to low frequenci..."
- 11:4711:47, 22 May 2025 diff hist 0 N File:496f2.png No edit summary current
- 11:4611:46, 22 May 2025 diff hist 0 N File:496f1.png No edit summary current
- 10:4710:47, 22 May 2025 diff hist +4 SolarNuggets No edit summary
11 May 2025
- 12:1112:11, 11 May 2025 diff hist +259 SolarNuggets No edit summary
- 12:0612:06, 11 May 2025 diff hist 0 N File:Icon495.png No edit summary current
- 08:0408:04, 11 May 2025 diff hist +814 A Multi-Site Telescope for Multi-Height for Synoptic Observations →The GATES network current
- 07:5007:50, 11 May 2025 diff hist +49 A Multi-Site Telescope for Multi-Height for Synoptic Observations →Conclusions
- 07:4907:49, 11 May 2025 diff hist +609 A Multi-Site Telescope for Multi-Height for Synoptic Observations author's corrections
- 07:3707:37, 11 May 2025 diff hist 0 N File:495f3.png No edit summary current
- 07:3407:34, 11 May 2025 diff hist +16 A Multi-Site Telescope for Multi-Height for Synoptic Observations →The GATES network
- 07:3307:33, 11 May 2025 diff hist +14 A Multi-Site Telescope for Multi-Height for Synoptic Observations →Observatories
- 07:2407:24, 11 May 2025 diff hist +3,433 N A Multi-Site Telescope for Multi-Height for Synoptic Observations Created page with "{{Infobox Nugget |name = Nugget |title = Multi-Height Multi-site Synoptic Observations |number = 495 |first_author = Fallon KONOW |publish_date = May 12, 2025 |next_nugget = |previous_nugget = {{#ask: Category:Nugget RHESSI Nugget Index::494}} }} == Introduction == We do not have adequate synoptic observations of the Sun at high cadence and high resolution. Such observations, especially if aimed at sampling multiple heights in the solar atmosphere, fill a..."
9 May 2025
- 08:1708:17, 9 May 2025 diff hist +3,433 N Multi-Height Multi-site Synoptic Observations No. 495 initial upload current
- 08:1608:16, 9 May 2025 diff hist 0 N File:495f2.png No edit summary current
- 08:1608:16, 9 May 2025 diff hist 0 N File:495f1.png No edit summary current
1 May 2025
- 15:0815:08, 1 May 2025 diff hist +4 SolarNuggets No edit summary
- 15:0715:07, 1 May 2025 diff hist 0 SolarNuggets No edit summary
24 April 2025
- 13:0113:01, 24 April 2025 diff hist +308 SolarNuggets Added No. 494
- 12:0012:00, 24 April 2025 diff hist 0 N File:Icon494.png No edit summary current
- 11:5611:56, 24 April 2025 diff hist 0 On turbulent magnetic reconnection: fast and slow mean steady-states →Steady states current
- 11:5511:55, 24 April 2025 diff hist 0 On turbulent magnetic reconnection: fast and slow mean steady-states →Steady states
- 11:5511:55, 24 April 2025 diff hist 0 On turbulent magnetic reconnection: fast and slow mean steady-states →Steady states
22 April 2025
- 19:5719:57, 22 April 2025 diff hist +5,507 N On turbulent magnetic reconnection: fast and slow mean steady-states No. 494 initial upload
- 19:5519:55, 22 April 2025 diff hist 0 File:494f2.png Hhudson uploaded a new version of File:494f2.png current
- 19:5319:53, 22 April 2025 diff hist 0 N File:494f2.png No edit summary
- 19:5319:53, 22 April 2025 diff hist 0 N File:494f1.png No edit summary current
17 April 2025
- 11:3511:35, 17 April 2025 diff hist −36 SolarNuggets No edit summary
- 11:3411:34, 17 April 2025 diff hist +289 SolarNuggets No edit summary
- 11:3011:30, 17 April 2025 diff hist 0 N File:Icon493.png No edit summary current
- 11:2011:20, 17 April 2025 diff hist +30 Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV author's fixes current
- 09:3809:38, 17 April 2025 diff hist 0 Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV No 493 figures
- 09:3609:36, 17 April 2025 diff hist 0 N File:493f2.png No edit summary current
- 09:3609:36, 17 April 2025 diff hist 0 N File:493f1.png No edit summary current
- 09:3609:36, 17 April 2025 diff hist 0 N File:493f34.png No edit summary current
- 09:3309:33, 17 April 2025 diff hist +5,621 N Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV No. 493
9 April 2025
- 09:2209:22, 9 April 2025 diff hist −7 SolarNuggets No edit summary
- 09:1809:18, 9 April 2025 diff hist 0 N File:Icon492.png No edit summary current
- 09:1709:17, 9 April 2025 diff hist +317 SolarNuggets added 492
