Aeronomy of Extra-Solar Giant Planets

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33796

Title:	Aeronomy of Extra-Solar Giant Planets
Authors:	Yelle,Roger;Lammer,Helmut;Ip,Wing-Huen
Contributors:	天文研究所
Keywords:	SMALL ORBITAL DISTANCES;HOT JUPITERS;RADIO EMISSIONS;MAGNETIC-FIELD;TAU-BOOTIS;KILOMETRIC RADIATION;EXOPLANET HD-209458B;HYDRODYNAMIC ESCAPE;ATMOSPHERIC LOSS;HD 209458B
Date:	2008
Issue Date:	2010-07-07 11:48:49 (UTC+8)
Publisher:	中央大學
Abstract:	The intense stellar UV radiation field incident upon extra-solar giant planets causes profound changes to their upper atmospheres. Upper atmospheric temperatures can be tens of thousands of kelvins, causing thermal dissociation of H-2 to H. The stellar io
Relation:	SPACE SCIENCE REVIEWS
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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