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In the model, the slots are mostly filled with water, and Saturn tides drive turbulent water flow in the slots whose dissipation produces enough heat to keep slots open. In turn, long-lived water-filled slots drive a volcano-tectonic feedback that buffers the rate of volcanism to approximately the observed value. Our results suggest that the ocean\u2013surface connection on Enceladus may be sustained on million-year timescales.<\/jats:p>","DOI":"10.1073\/pnas.1520507113","type":"journal-article","created":{"date-parts":[[2016,3,28]],"date-time":"2016-03-28T22:48:48Z","timestamp":1459205328000},"page":"3972-3975","update-policy":"https:\/\/doi.org\/10.1073\/pnas.cm10313","source":"Crossref","is-referenced-by-count":95,"title":["Sustained eruptions on Enceladus explained by turbulent dissipation in tiger stripes"],"prefix":"10.1073","volume":"113","author":[{"given":"Edwin S.","family":"Kite","sequence":"first","affiliation":[{"name":"Department of Geophysical Sciences, University of Chicago, Chicago, IL 60637;"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Allan M.","family":"Rubin","sequence":"additional","affiliation":[{"name":"Department of Geosciences, Princeton University, Princeton, NJ 08544"}],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"341","published-online":{"date-parts":[[2016,3,28]]},"reference":[{"key":"e_1_3_3_1_2","doi-asserted-by":"publisher","DOI":"10.1088\/0004-6256\/148\/3\/45"},{"key":"e_1_3_3_2_2","doi-asserted-by":"publisher","DOI":"10.1029\/2011GL047415"},{"key":"e_1_3_3_3_2","doi-asserted-by":"crossref","first-page":"A10204","DOI":"10.1029\/2011JA016693","article-title":"The water vapor plumes of Enceladus","volume":"116","author":"Dong Y","year":"2011","unstructured":"Y Dong, TW Hill, BD Teolis, BA Magee, JH Waite, The water vapor plumes of Enceladus. 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