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A universal model for solar eruptions

Author

Listed:
  • Peter F. Wyper

    (Durham University)

  • Spiro K. Antiochos

    (NASA Goddard Space Flight Center)

  • C. Richard DeVore

    (NASA Goddard Space Flight Center)

Abstract

Simulations of a solar coronal jet driven by filament ejection demonstrate that magnetic reconnection underlies the energy release, implying that a universal ‘breakout’ model explains both tiny jets and huge mass ejections from the Sun.

Suggested Citation

  • Peter F. Wyper & Spiro K. Antiochos & C. Richard DeVore, 2017. "A universal model for solar eruptions," Nature, Nature, vol. 544(7651), pages 452-455, April.
    • Handle: RePEc:nat:nature:v:544:y:2017:i:7651:d:10.1038_nature22050
    DOI: 10.1038/nature22050
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    Cited by:

    1. Pankaj Kumar & Valery M. Nakariakov & Judith T. Karpen & Kyung-Suk Cho, 2024. "Direct imaging of magnetohydrodynamic wave mode conversion near a 3D null point on the sun," Nature Communications, Nature, vol. 15(1), pages 1-11, December.

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