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Kliem, B · 2014 · DOI 10.1088/0004-637x/789/1/46

2 Pith papers cite this work. Polarity classification is still indexing.

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astro-ph.SR 2

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2026 2

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UNVERDICTED 2

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representative citing papers

Data-inspired simulation of AR 11158

astro-ph.SR · 2026-06-24 · unverdicted · novelty 5.0

Data-driven simulation of AR 11158 produces an X-flare triggered by torus instability after MFR formation above a cPIL, with energy release and photospheric changes matching some observed trends.

Effects of the Background Magnetic Field on Flux Rope Eruptions

astro-ph.SR · 2026-06-17 · unverdicted · novelty 4.0

Background magnetic field orientation affects eruption success and reconnection in MHD simulations of pre-existing flux ropes, with antiparallel fields enabling faster but shorter flare reconnection.

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Showing 2 of 2 citing papers after filters.

  • Data-inspired simulation of AR 11158 astro-ph.SR · 2026-06-24 · unverdicted · none · ref 25

    Data-driven simulation of AR 11158 produces an X-flare triggered by torus instability after MFR formation above a cPIL, with energy release and photospheric changes matching some observed trends.

  • Effects of the Background Magnetic Field on Flux Rope Eruptions astro-ph.SR · 2026-06-17 · unverdicted · none · ref 30

    Background magnetic field orientation affects eruption success and reconnection in MHD simulations of pre-existing flux ropes, with antiparallel fields enabling faster but shorter flare reconnection.