E. Hauri, E. Cottrell, Katherine A. Kelley, J. Tucker, K. Shimizu, M. L. Voyer, J. Marske, A. Saal
{"title":"对流地幔中的碳","authors":"E. Hauri, E. Cottrell, Katherine A. Kelley, J. Tucker, K. Shimizu, M. L. Voyer, J. Marske, A. Saal","doi":"10.1017/9781108677950.009","DOIUrl":null,"url":null,"abstract":"melt inclusions. This provides independent evidence that the MORB source is not graphite saturated; however, these curves could be relevant when considering more reduced planetary bodies, such as Mars.","PeriodicalId":146724,"journal":{"name":"Deep Carbon","volume":"84 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"17","resultStr":"{\"title\":\"Carbon in the Convecting Mantle\",\"authors\":\"E. Hauri, E. Cottrell, Katherine A. Kelley, J. Tucker, K. Shimizu, M. L. Voyer, J. Marske, A. Saal\",\"doi\":\"10.1017/9781108677950.009\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"melt inclusions. This provides independent evidence that the MORB source is not graphite saturated; however, these curves could be relevant when considering more reduced planetary bodies, such as Mars.\",\"PeriodicalId\":146724,\"journal\":{\"name\":\"Deep Carbon\",\"volume\":\"84 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"17\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Deep Carbon\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1017/9781108677950.009\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Deep Carbon","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1017/9781108677950.009","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
melt inclusions. This provides independent evidence that the MORB source is not graphite saturated; however, these curves could be relevant when considering more reduced planetary bodies, such as Mars.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
