Can an Unobserved Concentration of Magnetic Flux Above the Poles of the Sun Resolve the Open Flux Problem?

Global models of the extended solar corona, driven by observed photospheric magnetic fields, generally cannot reproduce the amplitude of the measured interplanetary magnetic field at 1 au (or elsewhere in the heliosphere), often underestimating it by a factor of two or more. Some modelers have attem...

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Veröffentlicht in:	The Astrophysical journal Jg. 884; H. 1; S. 18 - 29
Hauptverfasser:	Riley, Pete, Linker, Jon A., Mikic, Zoran, Caplan, Ronald M., Downs, Cooper, Thumm, Jean-Luc
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 10.10.2019 IOP Publishing
Schlagworte:	Astrophysics Computational fluid dynamics Corona Coronal holes Fluctuations Fluid flow Ground-based observation Heliosphere Interplanetary magnetic field Interplanetary magnetic fields Latitude Magnetic fields Magnetic flux Magnetohydrodynamic models Magnetohydrodynamical simulations Magnetohydrodynamics Observatories Photosphere Photospheric magnetic fields Potential fields Solar corona Solar coronal holes Solar coronal streamers Solar magnetic field Solar Orbiter (ESA) Solar orbits Solar photosphere Spacecraft Sun
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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