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本論文では惑星の固有磁場を構成する流体がどのように近似されるか調べた. 

その結果, 地球外核の流体の物性値や地球の諸物理量から\ MHD\ 近似とブシネスク近似が成り立つことが示された.
最後にこの流体力学の熱に関するスケールと電磁気学の磁場の拡散に関するスケールを無次元化し,\ 磁気拡散に比べ熱拡散が大きいことが示された.\ 


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