Simulations find that chromospheric three-minute oscillations arise from both direct upward propagation of three-minute waves and resonant trapping, with both requiring photospheric three-minute power and the resonator enhancing it under certain conditions.
C., Khomenko, E., & Collados, M
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Origin of the chromospheric three-minute oscillations in sunspot umbrae
Simulations find that chromospheric three-minute oscillations arise from both direct upward propagation of three-minute waves and resonant trapping, with both requiring photospheric three-minute power and the resonator enhancing it under certain conditions.