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02493nam a22004335i 4500 |
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|a 9783319633510
|9 978-3-319-63351-0
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|a 10.1007/978-3-319-63351-0
|2 doi
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|d GrThAP
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|a Chadney, Joshua.
|e author.
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|a Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars
|h [electronic resource] /
|c by Joshua Chadney.
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|a Cham :
|b Springer International Publishing :
|b Imprint: Springer,
|c 2017.
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|a XII, 169 p. 85 illus., 70 illus. in color.
|b online resource.
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|a text
|b txt
|2 rdacontent
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|a computer
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|2 rdamedia
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|a online resource
|b cr
|2 rdacarrier
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|a text file
|b PDF
|2 rda
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|a Springer Theses, Recognizing Outstanding Ph.D. Research,
|x 2190-5053
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|a 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.
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|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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|a Physics.
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|a Atmospheric sciences.
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|a Astrophysics.
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|a Physics.
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|a Planetary Sciences.
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|a Atmospheric Sciences.
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|a Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
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|a Astrophysics and Astroparticles.
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|a SpringerLink (Online service)
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|t Springer eBooks
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|i Printed edition:
|z 9783319633503
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|a Springer Theses, Recognizing Outstanding Ph.D. Research,
|x 2190-5053
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|u http://dx.doi.org/10.1007/978-3-319-63351-0
|z Full Text via HEAL-Link
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|a ZDB-2-PHA
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|a Physics and Astronomy (Springer-11651)
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