A STEADY-STATE PICTURE OF SOLAR WIND ACCELERATION AND CHARGE STATE COMPOSITION DERIVED FROM A GLOBAL WAVE-DRIVEN MHD MODEL

ABSTRACT The higher charge states found in slow (

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Bibliographic Details
Published in:The Astrophysical journal 2015-06, Vol.806 (1), p.1-25
Main Authors: Oran, R., Landi, E., Holst, B. van der, Lepri, S. T., Vásquez, A. M., Nuevo, F. A., Frazin, R., Manchester, W., Sokolov, I., Gombosi, T. I.
Format: Article
Language:English
Subjects:
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Charge
CHARGE STATES
COMPARATIVE EVALUATIONS
Coronal hole boundaries
ELECTRON DENSITY
EXTREME ULTRAVIOLET RADIATION
HELIOSPHERE
HYPOTHESIS
IONIZATION
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
magnetohydrodynamics (MHD)
MATHEMATICAL EVOLUTION
Mathematical models
methods: numerical
MHD
SOLAR CORONA
SOLAR WIND
STAR MODELS
STEADY-STATE CONDITIONS
Streams
SUN
Sun: corona
Sun: heliosphere
techniques: spectroscopic
TURBULENCE
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Description
Summary:ABSTRACT The higher charge states found in slow (
ISSN:0004-637X
1538-4357
1538-4357
DOI:10.1088/0004-637X/806/1/55