{"title":"关于湍流磁重联:快慢平均稳态","authors":"Sage Stanish, David MacTaggart","doi":"arxiv-2409.07346","DOIUrl":null,"url":null,"abstract":"We investigate a model of turbulent magnetic reconnection introduced by Yokoi\nand collaborators (Phys. Rev. Lett. 110, 255001) and show that the classic\ntwo-dimensional, steady-state Sweet-Parker and Petschek reconnection solutions\nare supported. We present evidence that these are the only two steady-state\nreconnection solutions, and we determine the criterion for their selection.\nSweet-Parker reconnection occurs when there is no growth in turbulent energy,\nwhereas Petschek reconnection occurs when the current density in the\nreconnecting current sheet is able to surpass a critical value, allowing for\nthe growth of turbulent energy that creates the diffusion region. Further, we\nshow that the Petschek solutions are self-similar, depending on the value of\nthe turbulent time scale. The self-consistent development of Petschek\nreconnection through turbulence, within the model, is an example of fast and\nsteady magnetic reconnection without an explicit need for the collisionless\nterms in an extended Ohm's law.","PeriodicalId":501274,"journal":{"name":"arXiv - PHYS - Plasma Physics","volume":"24 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"On turbulent magnetic reconnection: fast and slow mean steady-states\",\"authors\":\"Sage Stanish, David MacTaggart\",\"doi\":\"arxiv-2409.07346\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We investigate a model of turbulent magnetic reconnection introduced by Yokoi\\nand collaborators (Phys. Rev. Lett. 110, 255001) and show that the classic\\ntwo-dimensional, steady-state Sweet-Parker and Petschek reconnection solutions\\nare supported. We present evidence that these are the only two steady-state\\nreconnection solutions, and we determine the criterion for their selection.\\nSweet-Parker reconnection occurs when there is no growth in turbulent energy,\\nwhereas Petschek reconnection occurs when the current density in the\\nreconnecting current sheet is able to surpass a critical value, allowing for\\nthe growth of turbulent energy that creates the diffusion region. Further, we\\nshow that the Petschek solutions are self-similar, depending on the value of\\nthe turbulent time scale. The self-consistent development of Petschek\\nreconnection through turbulence, within the model, is an example of fast and\\nsteady magnetic reconnection without an explicit need for the collisionless\\nterms in an extended Ohm's law.\",\"PeriodicalId\":501274,\"journal\":{\"name\":\"arXiv - PHYS - Plasma Physics\",\"volume\":\"24 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Plasma Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.07346\",\"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 - PHYS - Plasma Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.07346","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
On turbulent magnetic reconnection: fast and slow mean steady-states
We investigate a model of turbulent magnetic reconnection introduced by Yokoi
and collaborators (Phys. Rev. Lett. 110, 255001) and show that the classic
two-dimensional, steady-state Sweet-Parker and Petschek reconnection solutions
are supported. We present evidence that these are the only two steady-state
reconnection solutions, and we determine the criterion for their selection.
Sweet-Parker reconnection occurs when there is no growth in turbulent energy,
whereas Petschek reconnection occurs when the current density in the
reconnecting current sheet is able to surpass a critical value, allowing for
the growth of turbulent energy that creates the diffusion region. Further, we
show that the Petschek solutions are self-similar, depending on the value of
the turbulent time scale. The self-consistent development of Petschek
reconnection through turbulence, within the model, is an example of fast and
steady magnetic reconnection without an explicit need for the collisionless
terms in an extended Ohm's law.