{"title":"导电流体介质湍流 MHD 模型的热力学构建","authors":"A. V. Kolesnichenko","doi":"10.1134/S0038094623070055","DOIUrl":null,"url":null,"abstract":"<p><b>Abstract</b>—In this article, a closed system of magnetohydrodynamic (MHD) equations on the mean flow scales, which is intended for simulating turbulent flows of electroconductive media in the presence of an electromagnetic field, is derived in the single-fluid MHD approximation.</p>","PeriodicalId":778,"journal":{"name":"Solar System Research","volume":"57 7","pages":"706 - 726"},"PeriodicalIF":0.6000,"publicationDate":"2024-03-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Thermodynamic Construction of the MHD Model of Turbulence of Electroconductive Fluid Medium\",\"authors\":\"A. V. Kolesnichenko\",\"doi\":\"10.1134/S0038094623070055\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><b>Abstract</b>—In this article, a closed system of magnetohydrodynamic (MHD) equations on the mean flow scales, which is intended for simulating turbulent flows of electroconductive media in the presence of an electromagnetic field, is derived in the single-fluid MHD approximation.</p>\",\"PeriodicalId\":778,\"journal\":{\"name\":\"Solar System Research\",\"volume\":\"57 7\",\"pages\":\"706 - 726\"},\"PeriodicalIF\":0.6000,\"publicationDate\":\"2024-03-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Solar System Research\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S0038094623070055\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar System Research","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0038094623070055","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Thermodynamic Construction of the MHD Model of Turbulence of Electroconductive Fluid Medium
Abstract—In this article, a closed system of magnetohydrodynamic (MHD) equations on the mean flow scales, which is intended for simulating turbulent flows of electroconductive media in the presence of an electromagnetic field, is derived in the single-fluid MHD approximation.
期刊介绍：
Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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