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Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse

Seven different models are applied to the same problem of simulating the Sun’s coronal magnetic field during the solar eclipse on 2015 March 20. All of the models are non-potential, allowing for free magnetic energy, but the associated electric currents are developed in significantly different ways....

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Dades bibliogràfiques
Publicat a:Space Sci Rev
Autors principals: Yeates, Anthony R., Amari, Tahar, Contopoulos, Ioannis, Feng, Xueshang, Mackay, Duncan H., Mikić, Zoran, Wiegelmann, Thomas, Hutton, Joseph, Lowder, Christopher A., Morgan, Huw, Petrie, Gordon, Rachmeler, Laurel A., Upton, Lisa A., Canou, Aurelien, Chopin, Pierre, Downs, Cooper, Druckmüller, Miloslav, Linker, Jon A., Seaton, Daniel B., Török, Tibor
Format: Artigo
Idioma:Inglês
Publicat: 2018
Matèries:
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC7493006/
https://ncbi.nlm.nih.gov/pubmed/32943800
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1007/s11214-018-0534-1
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