初期火星大気を想定した主成分凝結対流の二次元数値実験 : 臨界飽和比と凝結核数混合比に対する依存性 [論文内容及び審査の要旨]


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Tatsuya_Yamashita_abstract.pdf	論文内容の要旨	93.92 kB	PDF	View/Open
Tatsuya_Yamashita_review.pdf	審査の要旨	193.46 kB	PDF	View/Open

Please use this identifier to cite or link to this item:http://hdl.handle.net/2115/56685

Related Items in HUSCAP:

Title:	初期火星大気を想定した主成分凝結対流の二次元数値実験 : 臨界飽和比と凝結核数混合比に対する依存性 [論文内容及び審査の要旨]
Authors:	山下, 達也¹ Browse this author
Authors(alt):	YAMASHITA, Tatsuya¹
Issue Date:	30-Jun-2014
Publisher:	Hokkaido University
Conffering University:	北海道大学
Degree Report Number:	甲第11497号
Degree Level:	博士
Degree Discipline:	理学
Examination Committee Members:	(主査) 准教授石渡正樹, 教授倉本圭, 教授渡部重十, 教授高橋幸弘, 助教小高正嗣
Degree Affiliation:	理学院（宇宙理学専攻）
Rights:	http://creativecommons.org/licenses/by-nc-sa/2.1/jp/
Type:	theses (doctoral - abstract and summary of review)
URI:	http://hdl.handle.net/2115/56685
Appears in Collections:	学位論文 (Theses) > 博士　（理学）課程博士 (Doctorate by way of Advanced Course) > 理学院(Graduate School of Science)

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