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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Veröffentlicht in:	Space science reviews 2018-08, Vol.214 (5), p.1-27
Hauptverfasser:	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:	Artikel
Sprache:	eng
Schlagworte:	Activation Aerospace Technology and Astronautics Astrophysics and Astroparticles Boundary conditions Computer simulation Corona Coronal magnetic fields Electric currents Evolution Magnetic fields Photosphere Physics Physics and Astronomy Planetology Solar corona Solar eclipses Solar magnetic field Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Topology
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