<html><head><meta name="color-scheme" content="light dark"></head><body><pre style="word-wrap: break-word; white-space: pre-wrap;">% è¡¨é¡Œ  MHD ãƒ€ã‚¤ãƒŠãƒ¢ã®å®šå¼åŒ–
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\Dtitle{å›žè»¢çƒæ®» MHD ãƒ€ã‚¤ãƒŠãƒ¢ã®å®šå¼åŒ–}
\Dauthor{ä½ã€…æœ¨ æ´‹å¹³, ç«¹åºƒ çœŸä¸€, æž— ç¥¥ä»‹}
\Ddate{å¹³æˆ 14 å¹´ 10 æœˆ 4 æ—¥} 
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\section*{å‚è€ƒæ–‡çŒ®}
\addcontentsline{toc}{section}{å‚è€ƒæ–‡çŒ®}
\begin{description}
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\item Chandrasekhar,S.,1961: 
	    {\em Hydrodynamic and Hydromagnetic Stability}. 
	    Oxford University Press.
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\item Glatzmaier,G.A.,1984: 
	    Numerical simulations of stellar convective dynamos. 
	    {I}.the model and method. 
	    {\em J. Comput. Phys.},  {\bf 55}, 461--484.
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\item Hollerbach,R.,2000:
	    A spectral solution of the magneto-convection equations in
	    spherical geometry.
	    {\em J. Numer. Mech. Fluids},  {\bf 32}, 773-797.
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\item Zhang,K. and Busse,F.H.,1987: 
	    On the onset of convection in rotating spherical shells. 
	    {\em Geophys. Astrophys. Fluid Dyn.},  {\bf 39}, 119--147.
\end{description}
\end{document}



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