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

brachytherapy

書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars影響因子(影響力)




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars影響因子(影響力)學(xué)科排名




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars網(wǎng)絡(luò)公開度




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars被引頻次




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars被引頻次學(xué)科排名




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars年度引用




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars年度引用學(xué)科排名




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars讀者反饋




書目名稱Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars讀者反饋學(xué)科排名

BROOK

disrupt

978-3-319-87530-9Springer International Publishing AG 2017

圓桶

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

GRACE

Springer Theseshttp://image.papertrans.cn/m/image/636686.jpg

GRACE

SLAY

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

前兆

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

責(zé)問

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,

Platelet

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.?