Why are non-radial solar eruptions less frequent than radial ones?

Documenti analoghi

• 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)
• MHD simulations of the slow-rise phase of solar eruptions initiated from a sheared magnetic arcade
  di: Liu, Qingjun, et al.
  Pubblicazione: (2025)
• A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic Reconnection
  di: Liu, Qingjun, et al.
  Pubblicazione: (2024)
• On the analysis of eruptive events with non-radial evolution
  di: Sahade, Abril, et al.
  Pubblicazione: (2025)