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Cited article:

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Difference in the Characteristics of Solar Macrospicules at Low and High Latitudes

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Influence of Active Regions on Solar Wind Characteristics at the Cycle Maximum

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KORTES Mission for Solar Activity Monitoring Onboard International Space Station

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Can High-Mode Magnetohydrodynamic Waves Propagating in a Spinning Macrospicule Be Unstable Due to the Kelvin–Helmholtz Instability?

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Quasi-biennial oscillations in the cross-correlation of properties of macrospicules

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