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Showing below up to 47 results in range #1,251 to #1,297.

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  1. Solar Gamma-Ray Evidence for a Distinct Population of MeV Flare-Accelerated Electrons‏‎ (12:15, 5 February 2025)
  2. From Chromospheric Evaporation to Coronal Rain: An Investigation of the Mass and Energy Cycle of a Flare‏‎ (12:16, 5 February 2025)
  3. Energetic neutral atoms detected in the large solar energetic particle event of February 2022‏‎ (12:17, 5 February 2025)
  4. New insights into the proton precipitation sites in solar flares‏‎ (21:17, 6 February 2025)
  5. Advection and super-diffusive expansion as the model of flare accelerated electron transport in type III solar radio bursts‏‎ (20:56, 7 February 2025)
  6. Proton Beam Energy Deposition as a Mechanism of Deep Photospheric Heating‏‎ (20:14, 19 March 2025)
  7. Solar Rollercoaster: looping-the-loop in the solar corona‏‎ (21:35, 6 April 2025)
  8. Metis observations of Alfvenic outflows driven by interchange reconnection in a pseudostreamer‏‎ (09:14, 9 April 2025)
  9. Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV‏‎ (11:20, 17 April 2025)
  10. On turbulent magnetic reconnection: fast and slow mean steady-states‏‎ (11:56, 24 April 2025)
  11. Multi-Height Multi-site Synoptic Observations‏‎ (08:17, 9 May 2025)
  12. A Multi-Site Telescope for Multi-Height for Synoptic Observations‏‎ (08:04, 11 May 2025)
  13. Delay of Near-Relativistic Electrons‏‎ (14:46, 22 May 2025)
  14. The Sun's open-closed flux boundary and the origin of the slow solar wind‏‎ (06:52, 4 June 2025)
  15. High-Resolution Observations of a C3 class White-Light Flare‏‎ (08:52, 17 June 2025)
  16. Quasiperiodic Pulsations in the Balmer Continuum in an X-class Solar White-light Flare‏‎ (14:06, 2 July 2025)
  17. Five Hundred Nuggets‏‎ (07:18, 12 July 2025)
  18. Synchrotron Radiation and the Foundations for a Cosmic Bridge‏‎ (19:03, 30 August 2025)
  19. The Aulanier Effect: drifting footpoints of CME flux ropes‏‎ (19:04, 30 August 2025)
  20. Neupertianity‏‎ (09:49, 11 September 2025)
  21. Flare Phases and the Earth's Ionospheric Response‏‎ (19:56, 30 September 2025)
  22. SOLSTICE observes flare Doppler shifts in Si III‏‎ (08:31, 6 October 2025)
  23. Time evolution of flare-accelerated electrons in the warm-target model‏‎ (16:58, 14 October 2025)
  24. Time evolution of flare-accelerated electrons using the warm-target model‏‎ (13:05, 15 October 2025)
  25. FAI and GOES eclipses‏‎ (11:24, 30 October 2025)
  26. On the Origin of Solar Long-Duration Gamma-Ray Flares‏‎ (08:00, 5 November 2025)
  27. The EUV Late Phase‏‎ (08:38, 13 November 2025)
  28. Sun-as-a-star Analysis of a Solar Eruption Source Region Using H-alpha Spectroscopic Observations from CHASE‏‎ (21:45, 26 November 2025)
  29. Iron Fluorescence in X-class Solar Flares‏‎ (11:13, 15 December 2025)
  30. Spatial Distribution of Magnetic Reconnection Rate in an M6.5 Solar Flare‏‎ (12:40, 9 January 2026)
  31. Fine structures in solar flare ribbons‏‎ (17:44, 11 January 2026)
  32. The M- and X-class White-light Flares in Super Active Region NOAA 13664/13697‏‎ (17:46, 11 January 2026)
  33. On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona‏‎ (14:08, 14 January 2026)
  34. A fine-scale bright kernel captured by Hi-C 3 in the post-maximum phase of an M-class solar flare‏‎ (09:49, 10 February 2026)
  35. Observational Evidence Linking Loop Length and Thermal/Nonthermal Peak Timing in Solar Flares‏‎ (17:30, 27 February 2026)
  36. When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps‏‎ (09:48, 11 March 2026)
  37. Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Flare Loops‏‎ (20:20, 23 March 2026)
  38. How energetic can solar flares become?‏‎ (12:06, 29 March 2026)
  39. Can EUV Power-Spectral Indices Reveal Imminent Solar Flares?‏‎ (19:57, 13 April 2026)
  40. Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Nonradial to Radial Propagation‏‎ (09:29, 14 April 2026)
  41. An Unusual Long-Lived Radio Burst Oscillating in Frequency‏‎ (12:56, 22 April 2026)
  42. Observations of Slow Elemental Abundance Decay in Association to CME‏‎ (19:45, 22 April 2026)
  43. How Extreme Can Solar Flares Get? A Statistical View‏‎ (19:06, 5 May 2026)
  44. Space Weather Impact of Three Solar Flares Observed at Millimeter Wavelengths‏‎ (06:59, 26 May 2026)
  45. X-ray Log Letters‏‎ (11:07, 26 May 2026)
  46. White-Light and Lyman-alpha Emissions in Solar Flares: Timing, Timescale, Energy, and Scaling‏‎ (15:18, 4 June 2026)
  47. SolarNuggets‏‎ (19:15, 7 June 2026)

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