This work examines the convective instability of a horizontal layer of magnetohydrodynamic fluid of variable permeability when subjected to a non-vertical magnetic field. We use a model proposed by P.H. Roberts [9] in the context of neutron stars but the results obtained are also relevant to the area of ferromagnetic fluids. The presence of the variable permeability has no effect on the development of instabilities through the mechanism of stationary convection but influences the threshold of overstable convection which is often the preferred mechanism in non-terrestrial application. In the context of ferromagnetic fluids, both stationary and overstable instability can be expected to be realisable possibilities.
机构:
Univ Kebangsaan Malaysia, Fac Sci & Technol, Sch Math Sci, Bangi 43600, MalaysiaUniv Kebangsaan Malaysia, Fac Sci & Technol, Sch Math Sci, Bangi 43600, Malaysia
Arifin, NM
Hashim, I
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Univ Kebangsaan Malaysia, Fac Sci & Technol, Sch Math Sci, Bangi 43600, MalaysiaUniv Kebangsaan Malaysia, Fac Sci & Technol, Sch Math Sci, Bangi 43600, Malaysia
机构:
Jazan Univ, Math Dept, Sci Coll, POB 2097, Jazan 45142, Saudi ArabiaJazan Univ, Math Dept, Sci Coll, POB 2097, Jazan 45142, Saudi Arabia
Abasher, Abdelfatah
Ali, Elsiddeg
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Taif Univ, Turabah Univ Coll, Math Dept, PO Box 11099, Taif 21944, Saudi ArabiaJazan Univ, Math Dept, Sci Coll, POB 2097, Jazan 45142, Saudi Arabia
Ali, Elsiddeg
Adam, Hajer
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Jazan Univ, Coll Sci, Dept Phys, POB 114, Jazan 45142, Saudi ArabiaJazan Univ, Math Dept, Sci Coll, POB 2097, Jazan 45142, Saudi Arabia
Adam, Hajer
INTERNATIONAL JOURNAL OF ANALYSIS AND APPLICATIONS,
2024,
22