D. Graham, Y. Khotyaintsev, M. André, A. Vaivads, A. Chasapis, W. Matthaeus, A. Retinò, F. Valentini, D. Gershman
{"title":"地球磁层顶附近电子分布的非麦克斯韦性","authors":"D. Graham, Y. Khotyaintsev, M. André, A. Vaivads, A. Chasapis, W. Matthaeus, A. Retinò, F. Valentini, D. Gershman","doi":"10.1002/ESSOAR.10506282.1","DOIUrl":null,"url":null,"abstract":"Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibrium and deviate sig...","PeriodicalId":8461,"journal":{"name":"arXiv: Plasma Physics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2021-02-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"Non-Maxwellianity of electron distributions near Earth's magnetopause\",\"authors\":\"D. Graham, Y. Khotyaintsev, M. André, A. Vaivads, A. Chasapis, W. Matthaeus, A. Retinò, F. Valentini, D. Gershman\",\"doi\":\"10.1002/ESSOAR.10506282.1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibrium and deviate sig...\",\"PeriodicalId\":8461,\"journal\":{\"name\":\"arXiv: Plasma Physics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-02-19\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: Plasma Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1002/ESSOAR.10506282.1\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Plasma Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1002/ESSOAR.10506282.1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Non-Maxwellianity of electron distributions near Earth's magnetopause
Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibrium and deviate sig...
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
