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\chapter{はじめに}

\section{研究の目的}


火星の大気環境は, 地球と比較して極めて低温低圧で乾燥している. 
しかしながら, 赤道付近では昼間に 0 $^\circ$C 近くまで気温が上昇することに加え, 低圧のため昇華が促されるため H$_2$O の氷の維持が困難であると考えられるが,  
近年の観測で, 氷河に起因する特徴的な地形が確認されている. %参考文献？？
これは, 過去の火星において現在とは異なる気候の時期があったことを示唆している. 

このような低緯度の氷河地形が形成された当時の気候を解明する手がかりをつかむ方法の一つに, 数値シミュレーションによる気候再現がある. 
本研究では, 過去の気候変化を議論するための前段階として, まず現在の
火星条件下における大気環境を再現した.

\section{本論文の構成}

2 章では今回使用したモデルである DCPAM5 について述べ, 後半では今回の実験設定を紹介する. 
3 章ではシミュレーションの結果を出力した図を DCPAM5 の計算例や観測結果と比較する.  
4 章では 3 章で出力したデータの正当性を検証する. 

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