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{"id":54893,"date":"2021-03-31T13:47:00","date_gmt":"2021-03-31T12:47:00","guid":{"rendered":"https:\/\/www.lse.ac.uk\/granthaminstitute\/?post_type=publication&p=54893"},"modified":"2021-09-02T10:27:18","modified_gmt":"2021-09-02T09:27:18","slug":"magnetic-topology-of-actively-evolving-and-passively-convecting-structures-in-the-turbulent-solar-wind","status":"publish","type":"publication","link":"https:\/\/www.lse.ac.uk\/granthaminstitute\/publication\/magnetic-topology-of-actively-evolving-and-passively-convecting-structures-in-the-turbulent-solar-wind\/","title":{"rendered":"Magnetic Topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind"},"content":{"rendered":"\n

B. Hnat, S. C. Chapman, and N. W. Watkins. Magnetic Topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind, Phys. Rev. Lett<\/em>. 126, 125101<\/strong><\/p>\n\n","protected":false},"excerpt":{"rendered":"\n

Multipoint in situ observations of the solar wind are used to identify the magnetic topology and current density of turbulent structures. We find that at least 35% of all structures are both actively evolving and carrying the strongest currents, actively dissipating, and heating the plasma. <\/p>\n\n","protected":false},"author":12,"featured_media":0,"template":"","tags":[],"publication-type":[436],"topic_area":[],"class_list":["post-54893","publication","type-publication","status-publish","hentry","publication-type-research-articles"],"acf":{"exclude_from_sync":{"ref_value":"field_560538b0e7350","value":"0","type":false,"post_type":""},"downloads":{"ref_value":"field_52f16cc1a80f2","value":false,"type":"repeater","post_type":""},"rss_newsletter":{"ref_value":"field_54f5c2c1544d8","value":"","type":false,"post_type":""},"profile_link":{"ref_value":"field_52f164b5189e9","value":["nick-watkins"],"type":"relationship","post_type":"profile"},"article_link":{"ref_value":"field_52eee3c7f0586","value":"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.126.125101","type":false,"post_type":""},"article_link_title":{"ref_value":"field_5322399d89d42","value":"External link to article","type":false,"post_type":""},"spotlight":{"ref_value":"field_52f80896506d3","value":"","type":false,"post_type":""}},"yoast_head":"\nMagnetic Topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind - Grantham Research Institute on climate change and the environment<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.lse.ac.uk\/granthaminstitute\/publication\/magnetic-topology-of-actively-evolving-and-passively-convecting-structures-in-the-turbulent-solar-wind\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Magnetic Topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind - Grantham Research Institute on climate change and the environment\" \/>\n<meta property=\"og:description\" content=\"Multipoint in situ observations of the solar wind are used to identify the magnetic topology and current density of turbulent structures. 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