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Modelling the upper atmosphere of ga...

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Modelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Modelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars/ by Joshua Chadney.
作者:	Chadney, Joshua.
出版者:	Cham :Springer International Publishing : : 2017.,
面頁冊數:	xii, 169 p. :ill., digital ; : 24 cm.;
Contained By:	Springer eBooks
標題:	Extrasolar planets - Atmospheres -
電子資源:	http://dx.doi.org/10.1007/978-3-319-63351-0
ISBN:	9783319633510

Modelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars
Chadney, Joshua.

Modelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars[electronic resource] /by Joshua Chadney. - Cham :Springer International Publishing :2017. - xii, 169 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

1 Introduction -- 2 Solar and stellar X-ray and UV radiation -- 3 Thermosphere -- 4 Ionosphere -- 5 Conclusions and future work -- References -- Appendix A Neutral densities -- Appendix B Ion densities from the thermospheric model -- Appendix C Summary of permission for third party copyright works.

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.

ISBN: 9783319633510

Standard No.: 10.1007/978-3-319-63351-0doiSubjects--Topical Terms:

1199280
Extrasolar planets
--Atmospheres

LC Class. No.: QB820

Dewey Class. No.: 523.24

Modelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars
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520 $a 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.
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