MHD simulations of the slow-rise phase of solar eruptions initiated from a sheared magnetic arcade

Documenti analoghi

• Why are non-radial solar eruptions less frequent than radial ones?
  di: Liu, Qingjun, et al.
  Pubblicazione: (2024)
• An investigation of magnetic energy and helicity thresholds at the onset of solar eruptions based on numerical simulations
  di: Bian, Xinkai, et al.
  Pubblicazione: (2026)
• The role of photospheric magnetic flux diffusion in initiation of solar eruptions
  di: Bian, Xinkai, et al.
  Pubblicazione: (2025)
• Flux rope formation through flux cancellation of sheared coronal arcades in a 3D convectively-driven MHD simulation
  di: Furuseth, Sondre Vik, et al.
  Pubblicazione: (2025)
• Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption
  di: Xie, Xiaoyan, et al.
  Pubblicazione: (2025)