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.
E., Shibasaki, K., Sych, R
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.