A surface thermal model and exospheric ballistic transport code of planet Mercury

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33795

Title:	A surface thermal model and exospheric ballistic transport code of planet Mercury
Authors:	Wang,Y. -C.;Ip,W. -H.
Contributors:	天文研究所
Keywords:	ATMOSPHERE;SODIUM;MOON
Date:	2008
Issue Date:	2010-07-07 11:48:47 (UTC+8)
Publisher:	中央大學
Abstract:	The atmosphere of Mercury is of an exospheric nature. Its formation is due to several physical mechanisms including meteoroid impact, surface sputtering by solar wind ions and photon sputtering by solar UV radiation. The molecules and atoms emitted from t
Relation:	ADVANCES IN SPACE RESEARCH????
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

Files in This Item:

File	Description	Size	Format
index.html		0Kb	HTML	360	View/Open

社群 sharing