Multi-height data reveal a dominant standing sausage mode (~1-2 mHz) and a propagating fluting mode (m=2, ~2-3.5 mHz) in pore boundary oscillations, with the first mode carrying 66-86% of the eigenvalue power.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.SR 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
DKIST observations identify four-lobed Stokes U profiles as a potential signature of line-of-sight magnetic azimuth variation in sunspot penumbrae.
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.
citing papers explorer
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Multi-height Identification of Sausage and Fluting Eigenmodes in a Solar Pore
Multi-height data reveal a dominant standing sausage mode (~1-2 mHz) and a propagating fluting mode (m=2, ~2-3.5 mHz) in pore boundary oscillations, with the first mode carrying 66-86% of the eigenvalue power.
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DKIST Unveils Four-Lobed Stokes U Profiles in a Magnetically Complex Sunspot Penumbra
DKIST observations identify four-lobed Stokes U profiles as a potential signature of line-of-sight magnetic azimuth variation in sunspot penumbrae.
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Data-inspired simulation of AR 11158
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.