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Updated: Mar 3, 2026

X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells
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A universal model for solar eruptions.

Peter F Wyper1, Spiro K Antiochos2, C Richard DeVore2

  • 1Department of Mathematical Sciences, Durham University, Durham DH1 3LE, UK.

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|April 28, 2017
PubMed
Summary
This summary is machine-generated.

Solar eruptions, like coronal mass ejections and jets, may share a single origin. Simulations show magnetic breakout drives jets via reconnection, suggesting this mechanism underlies all solar eruptions.

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Area of Science:

  • Solar physics
  • Plasma astrophysics
  • Magnetohydrodynamics

Background:

  • Solar eruptions, including coronal mass ejections (CMEs) and coronal jets, involve the ejection of magnetized plasma from the Sun.
  • Traditionally, CMEs were thought to arise from ideal magnetohydrodynamic instabilities (e.g., kink or torus instability), while jets were attributed to magnetic reconnection.
  • Recent observations suggest coronal jets are also driven by filament ejection, similar to CMEs, implying a unified physical origin.

Purpose of the Study:

  • To investigate the underlying physical mechanism driving solar eruptions, specifically coronal jets.
  • To determine if a single mechanism, such as magnetic reconnection or ideal instability, can explain both jets and CMEs.
  • To test the hypothesis that filament ejection is a common driver for different scales of solar eruptions.

Main Methods:

  • Numerical simulations of a coronal jet driven by the eruption of a highly sheared magnetic flux rope (filament).
  • Analysis of the simulation results to identify the energy release process and magnetic topology changes.
  • Comparison of simulation outcomes with theoretical models and observational evidence for solar eruptions.

Main Results:

  • Simulations demonstrate that magnetic reconnection is the primary energy release mechanism during the simulated coronal jet.
  • The process observed is 'magnetic breakout,' a positive feedback loop between filament ejection and enhanced magnetic reconnection.
  • The results indicate that filament ejection, coupled with magnetic reconnection, can drive solar eruptions across different scales.

Conclusions:

  • Coronal jets driven by filament ejection are caused by magnetic reconnection via the magnetic breakout mechanism.
  • If coronal mass ejections and jets share a common physical origin, magnetic reconnection (specifically magnetic breakout) must be the universal mechanism.
  • The magnetic breakout model provides a unified explanation for the diverse range of magnetically driven solar eruptions.