Magnetic Field Variability as a Consistent Predictor of Solar Flares

Documenti analoghi

• 131 and 304 Å Emission Variability Increases Hours Prior to Solar Flare Onset
  di: Kniezewski, Kara L., et al.
  Pubblicazione: (2024)
• Statistical Overview of Long-Lived Active Regions Observed Across Multiple Carrington Rotations
  di: Mason, Emily I., et al.
  Pubblicazione: (2025)
• Survey of Magnetic Field Parameters Associated With Large Solar Flares
  di: Li, Ting, et al.
  Pubblicazione: (2024)
• Prediction of Large Solar Flares Based on SHARP and HED Magnetic Field Parameters
  di: Li, Xuebao, et al.
  Pubblicazione: (2024)
• Energetics and Emission in a Simulated Solar Flare Initialised by a Non-Force Free Magnetic Field
  di: Bate, W., et al.
  Pubblicazione: (2026)