Nonlinear magneto-hydrodynamical modeling of solar envelope
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Tarih
2006
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Amer Inst Physics
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
In this study, our objective was to investigate the variation of the physical parameters in the 30 % outermost convective solar layer with the use equations of magneto-hydrodynamics (MHD) for non-linear case. The anelastic approximation was used in our calculations. The variations in physical parameters were performed by Maple. Hydrostatics equilibrium state was taken as a Standard Solar Model (SSM) excluding both rotation and magnetic field.
Açıklama
7th International Conference of the Hellenic-Astronomical-Society -- SEP 08-11, 2006 -- Lixourion, GREECE
Anahtar Kelimeler
sun : magnetic fields : magneto-hydrodynamics, anelastic approximation
Kaynak
Recent Advances in Astronomy and Astrophysics
WoS Q Değeri
N/A
Scopus Q Değeri
Q4
Cilt
848
