{"title":"金星大气的热平衡","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":"{\"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}","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}
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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