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One type of leading theoretical models requires high-frequency magnetohydrodynamic (MHD) waves to transport and dissipate sufficient energy in the corona. However, such high-frequency waves with energetically significant amplitudes have never been unambiguously observed, leaving a key gap between theories and observations. Using high-cadence, high-resolution extreme-ultraviolet imaging from Solar Orbiter\u2019s Extreme Ultraviolet Imager, we identify a previously hidden population of high-frequency MHD waves in coronal plumes of the solar polar region. An analysis of the detected propagating kink waves shows that over one-third have periods shorter than 100\u00a0s, a population largely undetected by earlier instruments. Power spectral analysis demonstrates that these high-frequency waves carry substantial energy flux, which are significantly underestimated in lower-cadence data. These results suggest that high-frequency MHD waves may contribute importantly to the energy budget of the solar polar corona and could play a role in solar wind acceleration, highlighting the value of high-resolution observations for probing energy transport in magnetized space and astrophysical plasmas.<\/jats:p>","DOI":"10.1093\/nsr\/nwag370","type":"journal-article","created":{"date-parts":[[2026,6,16]],"date-time":"2026-06-16T12:28:23Z","timestamp":1781612903000},"source":"Crossref","is-referenced-by-count":1,"title":["High-frequency magnetohydrodynamic waves with substantial energy in the solar polar corona"],"prefix":"10.1093","volume":"13","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-6641-8034","authenticated-orcid":false,"given":"Yuhang","family":"Gao","sequence":"first","affiliation":[{"name":"School of Earth and Space Sciences, Peking University , Beijing, 100871 ,","place":["China"]},{"name":"State Key Laboratory of Solar Activity and Space Weather, National Space 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