{"title":"[Weizsäcker's cosmogony, Farm Hall and the origin of modern turbulence theory].","authors":"Michael Eckert","doi":"","DOIUrl":null,"url":null,"abstract":"<p><p>The modem statistical theory of turbulence was originated by Andrey Nikolaevich Kolmogorov (1903-1987), Lars Onsager (1903-1976), Ludwig Prandtl (1875-1953), Werner Heisenberg (1901-1976) und Carl Friedrich von Weizsäcker (1912-2007). With the exception of Kolmogorovs theory which was published in 1941 but became widely known only after the war, these contributions emerged largely independently from another in a \"remarkable series of coincidences\" (Batchelor 1946). Heisenberg and Weizäscker developed their theories during their detention at Farm Hall. Their work was motivated by von Weizsäcker's interest in astrophysics. Weizsäcker aimed at an understanding of the role of turbulence for the motion of interstellar matter for his theory about the origin of the planetary system which he had published in 1943. Weizsäcker's work on cosmogony and turbulence illustrates an early interaction between the disciplines of astronomy and fluid mechanics that became characteristic for astrophysics in the second half of the twentieth century.</p>","PeriodicalId":7006,"journal":{"name":"Acta historica Leopoldina","volume":" 63","pages":"101-16"},"PeriodicalIF":0.0000,"publicationDate":"2014-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta historica Leopoldina","FirstCategoryId":"1085","ListUrlMain":"","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The modem statistical theory of turbulence was originated by Andrey Nikolaevich Kolmogorov (1903-1987), Lars Onsager (1903-1976), Ludwig Prandtl (1875-1953), Werner Heisenberg (1901-1976) und Carl Friedrich von Weizsäcker (1912-2007). With the exception of Kolmogorovs theory which was published in 1941 but became widely known only after the war, these contributions emerged largely independently from another in a "remarkable series of coincidences" (Batchelor 1946). Heisenberg and Weizäscker developed their theories during their detention at Farm Hall. Their work was motivated by von Weizsäcker's interest in astrophysics. Weizsäcker aimed at an understanding of the role of turbulence for the motion of interstellar matter for his theory about the origin of the planetary system which he had published in 1943. Weizsäcker's work on cosmogony and turbulence illustrates an early interaction between the disciplines of astronomy and fluid mechanics that became characteristic for astrophysics in the second half of the twentieth century.
现代湍流统计理论是由Andrey Nikolaevich Kolmogorov (1903-1987), Lars Onsager (1903-1976), Ludwig Prandtl (1875-1953), Werner Heisenberg(1901-1976)和Carl Friedrich von Weizsäcker(1912-2007)创立的。除了柯尔莫哥罗夫的理论在1941年发表,但直到二战后才广为人知,这些贡献在很大程度上都是在“一系列显著的巧合”中独立出现的(Batchelor 1946)。海森堡和Weizäscker在他们被关押在农场大厅期间发展了他们的理论。冯Weizsäcker对天体物理学的兴趣激发了他们的工作。Weizsäcker的目标是理解星际物质运动中湍流的作用,这是他在1943年发表的关于行星系统起源的理论。Weizsäcker在宇宙学和湍流方面的工作说明了天文学和流体力学学科之间的早期相互作用,这种相互作用在20世纪下半叶成为天体物理学的特征。