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Titlebook: Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars; Joshua Chadney Book 2017 Springer International Publi

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发表于 2025-3-21 16:35:30 | 显示全部楼层 |阅读模式
书目名称Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars
编辑Joshua Chadney
视频video
概述Nominated as an outstanding PhD thesis by the Imperial College London, London, UK.Provides the description of upper atmospheric modeling on extrasolar giant planets (EGPs).Shows the calculation of esc
丛书名称Springer Theses
图书封面Titlebook: Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars;  Joshua Chadney Book 2017 Springer International Publi
描述This PhD thesis details the development of a new 1D ionospheric model to describe the upper atmospheres of extrasolar giant plants. The upper atmospheres of Hot Jupiters are subject to extreme radiation conditions that can result in rapid atmospheric escape. The composition and structure of these planets’ upper atmospheres are affected by high-energy emissions from the host star. The nature of these emissions depends on the stellar type and age, making them important factors in understanding the behaviour of exoplanetary atmospheres. 
出版日期Book 2017
关键词Exoplanetary Aeronomy; Exoplanetary Upper Atmosphere; Ionosphere; Thermosphere; Low-mass Stars; Exoplanet
版次1
doihttps://doi.org/10.1007/978-3-319-63351-0
isbn_softcover978-3-319-87530-9
isbn_ebook978-3-319-63351-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing AG 2017
The information of publication is updating

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发表于 2025-3-21 20:14:58 | 显示全部楼层
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978-3-319-87530-9Springer International Publishing AG 2017
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Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars978-3-319-63351-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
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Springer Theseshttp://image.papertrans.cn/m/image/636686.jpg
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2190-5053 ure of these emissions depends on the stellar type and age, making them important factors in understanding the behaviour of exoplanetary atmospheres. 978-3-319-87530-9978-3-319-63351-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
发表于 2025-3-22 22:57:12 | 显示全部楼层
2190-5053 extrasolar giant planets (EGPs).Shows the calculation of escThis PhD thesis details the development of a new 1D ionospheric model to describe the upper atmospheres of extrasolar giant plants. The upper atmospheres of Hot Jupiters are subject to extreme radiation conditions that can result in rapid a
发表于 2025-3-23 02:25:30 | 显示全部楼层
Book 2017res of Hot Jupiters are subject to extreme radiation conditions that can result in rapid atmospheric escape. The composition and structure of these planets’ upper atmospheres are affected by high-energy emissions from the host star. The nature of these emissions depends on the stellar type and age,
发表于 2025-3-23 07:15:46 | 显示全部楼层
Book 2017anets’ upper atmospheres are affected by high-energy emissions from the host star. The nature of these emissions depends on the stellar type and age, making them important factors in understanding the behaviour of exoplanetary atmospheres. 
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