Oldest pages

Jump to navigation Jump to search

Showing below up to 50 results in range #1,101 to #1,150.

View ( | ) (20 | 50 | 100 | 250 | 500)

  1. Cosmic Rays over the Rainbow Bridge‏‎ (15:09, 19 December 2019)
  2. Observational evidence for breakout reconnection‏‎ (10:58, 26 December 2019)
  3. A Global Survey of EUV Coronal Power Spectra‏‎ (16:46, 31 December 2019)
  4. Remembering John Brown‏‎ (20:16, 21 January 2020)
  5. A PSP Perihelion‏‎ (20:38, 2 February 2020)
  6. The Temporal and Spatial Extension of Gamma-ray Emission from the Sun‏‎ (17:22, 19 February 2020)
  7. A Hot Cusp-Shaped Confined Solar Flare‏‎ (20:11, 23 February 2020)
  8. Heating of the solar photosphere during a white-light flare‏‎ (12:15, 25 February 2020)
  9. The M5.5 Solar Flare on September 4, 2017 as a Source of Relativistic Electrons and Protons‏‎ (20:21, 12 March 2020)
  10. SOL2017-09-04 (M5.5) 2017 as a Source of Relativistic Electrons and Protons‏‎ (16:25, 21 March 2020)
  11. Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth‏‎ (19:57, 8 April 2020)
  12. Using overlappogram data to find hot flare plasma‏‎ (14:58, 17 April 2020)
  13. Phenomena in the unusually long pre-impulsive phase of SOL2011-06-07‏‎ (14:34, 18 April 2020)
  14. Broad symmetrical Doppler-shifted Fe XXI line profiles‏‎ (20:32, 28 April 2020)
  15. Rejuvenating Solar Flare Termination Shocks as Particle Accelerators‏‎ (09:52, 8 May 2020)
  16. Quasi-periodic pulsations as indicators of oscillatory processes in solar flares‏‎ (10:21, 10 May 2020)
  17. Test-2020-09-11‏‎ (08:08, 11 September 2020)
  18. Gregp-test-2020-09-11‏‎ (20:15, 11 September 2020)
  19. Test https://‏‎ (20:41, 11 September 2020)
  20. SOL2013-11-10 Eruptive Circular-ribbon Flare with Extended Remote Brightenings‏‎ (08:44, 15 September 2020)
  21. Extreme-Ultraviolet Late Phase of Solar Flares‏‎ (09:20, 15 September 2020)
  22. Gregp-test-2020-09-14‏‎ (15:44, 15 September 2020)
  23. Energy transport by accelerated particles in the quiet solar atmosphere‏‎ (07:00, 17 September 2020)
  24. Sunspot Differential Rotation in an X-class Flare‏‎ (13:26, 17 September 2020)
  25. Energy Partitioning in a Nonthermally Dominated Two-loop Solar Flare‏‎ (06:23, 18 September 2020)
  26. Relation of Non-neutralized electric currents and the activity in active regions‏‎ (13:18, 25 September 2020)
  27. Circular Ribbon Flare at Microwaves‏‎ (14:09, 2 October 2020)
  28. Submerged Flare Acoustic Sources‏‎ (20:43, 13 October 2020)
  29. Test-20201018‏‎ (18:56, 18 October 2020)
  30. Prediction of Solar Cycle 25‏‎ (08:58, 19 October 2020)
  31. Electric Current Neutralization and Eruption‏‎ (15:43, 19 October 2020)
  32. Flare/CME Cartoon Archive‏‎ (08:27, 26 October 2020)
  33. FLUKA as a tool for modelling gamma-ray production in flarres‏‎ (11:49, 2 November 2020)
  34. Valderrama in the 21st Century‏‎ (13:43, 3 November 2020)
  35. Hot Flare Onsets‏‎ (16:18, 16 November 2020)
  36. Self-Consistent Flare Model‏‎ (12:51, 17 November 2020)
  37. Probing the solar coronal heating function with slow magnetoacoustic waves‏‎ (16:41, 21 November 2020)
  38. What drives impulsive coronal heating?‏‎ (08:29, 25 November 2020)
  39. White-light emission and photospheric magnetic field changes in flares‏‎ (14:06, 25 November 2020)
  40. Investigation of Small-Scale Energy Releases in Hard X-rays with ​FOXSI‏‎ (11:13, 6 December 2020)
  41. Solar effects in the local interstellar medium‏‎ (16:22, 31 December 2020)
  42. Observing Solar Flare X-ray Polarization with Prospective CubeSat Missions‏‎ (16:34, 7 January 2021)
  43. Richard Schwartz‏‎ (20:22, 21 February 2021)
  44. A Collective Study of 11 NuSTAR Microflares‏‎ (20:19, 24 February 2021)
  45. NuSTAR Observations of 11 Microflares‏‎ (20:19, 24 February 2021)
  46. FLUKA as a tool for interpreting flare gamma-rays‏‎ (12:28, 28 February 2021)
  47. The Neupert Effect Revisited‏‎ (12:23, 4 March 2021)
  48. A Solar FRB‏‎ (20:57, 10 March 2021)
  49. The Superflare SOL2017-09-06: from submm to mid-IR‏‎ (20:49, 18 March 2021)
  50. Flare waiting times depend on their magnitudes‏‎ (08:12, 24 March 2021)

View ( | ) (20 | 50 | 100 | 250 | 500)