{"title":"THE THERMAL BALANCE OF THE VENUS ATMOSPHERE","authors":"D. Crisp, D. Titov","doi":"10.2307/j.ctv27tct5m.16","DOIUrl":null,"url":null,"abstract":"Observations of the Venus thermal structure colledted during the first three decades of the space age reveal high surface temperatures, near-adiabatic vertical temperature gradients throughout the lower atmosphere, and a reversed pol-to-equator mesospheric thermal structure, with polar temperatures that are higher than those over the equator.","PeriodicalId":409969,"journal":{"name":"Venus II","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2022-02-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"22","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Venus II","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2307/j.ctv27tct5m.16","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 22
Abstract
Observations of the Venus thermal structure colledted during the first three decades of the space age reveal high surface temperatures, near-adiabatic vertical temperature gradients throughout the lower atmosphere, and a reversed pol-to-equator mesospheric thermal structure, with polar temperatures that are higher than those over the equator.
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