{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,10,23]],"date-time":"2026-10-23T23:24:35Z","timestamp":1792797875220,"version":"4.5.0"},"reference-count":55,"publisher":"American Association for the Advancement of Science (AAAS)","issue":"6489","funder":[{"name":"JSPS","award":["16H02231"],"award-info":[{"award-number":["16H02231"]}]},{"name":"JSPS","award":["16H02225"],"award-info":[{"award-number":["16H02225"]}]},{"name":"JSPS","award":["19H05605"],"award-info":[{"award-number":["19H05605"]}]},{"name":"JSPS","award":["19K14789"],"award-info":[{"award-number":["19K14789"]}]},{"name":"JSPS","award":["16H02231"],"award-info":[{"award-number":["16H02231"]}]},{"name":"nasa hq","award":["NNX16AC79G"],"award-info":[{"award-number":["NNX16AC79G"]}]},{"name":"International Top Young Fellowship"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Science"],"published-print":{"date-parts":[[2020,4,24]]},"abstract":"<jats:title>Explaining super-rotation on Venus<\/jats:title>\n                  <jats:p>\n                    The solid surface of Venus rotates very slowly, once every 243 days, but its thick atmosphere circles the planet in just 4 days. This phenomenon, known as super-rotation, requires a continuous input of angular momentum, from an unknown source, to overcome friction with the surface. Horinouchi\n                    <jats:italic>et al.<\/jats:italic>\n                    mapped the planet's winds using ultraviolet observations of Venus' clouds from the orbiting Akatsuki spacecraft (see the Perspective by Lebonnois). They incorporated these data into a global model of angular momentum transport in the atmosphere, finding that the super-rotation is maintained through thermal tides driven by solar heating.\n                  <\/jats:p>\n                  <jats:p>\n                    <jats:italic>Science<\/jats:italic>\n                    , this issue p.\n                    <jats:related-article xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" ext-link-type=\"doi\" issue=\"6489\" page=\"405\" related-article-type=\"in-this-issue\" vol=\"368\" xlink:href=\"10.1126\/science.aaz4439\">405<\/jats:related-article>\n                    ; see also p.\n                    <jats:related-article xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" ext-link-type=\"doi\" issue=\"6489\" page=\"363\" related-article-type=\"in-this-issue\" vol=\"368\" xlink:href=\"10.1126\/science.abb2424\">363<\/jats:related-article>\n                  <\/jats:p>","DOI":"10.1126\/science.aaz4439","type":"journal-article","created":{"date-parts":[[2020,9,11]],"date-time":"2020-09-11T16:55:25Z","timestamp":1599843325000},"page":"405-409","source":"Crossref","is-referenced-by-count":67,"title":["How waves and turbulence maintain the super-rotation of Venus\u2019 atmosphere"],"prefix":"10.1126","volume":"368","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-2296-1975","authenticated-orcid":true,"given":"Takeshi","family":"Horinouchi","sequence":"first","affiliation":[{"name":"Faculty of Environmental Earth Science, Hokkaido University, Sapporo, Japan."},{"name":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-4745-4520","authenticated-orcid":true,"given":"Yoshi-Yuki","family":"Hayashi","sequence":"additional","affiliation":[{"name":"Department of Planetology and Center for Planetary 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