000796526 000__ 03780cam\a2200517M\\4500
000796526 001__ 796526
000796526 005__ 20230306143533.0
000796526 006__ m\\\\\o\\d\\\\\\\\
000796526 007__ cr\un\nnnunnun
000796526 008__ 170728s2017\\\\sz\\\\\\ob\\\\001\0\eng\d
000796526 019__ $$a994882836$$a996402146$$a999537173
000796526 020__ $$a9783319633510$$q(electronic book)
000796526 020__ $$a3319633511$$q(electronic book)
000796526 020__ $$z9783319633503
000796526 020__ $$z3319633503
000796526 035__ $$aSP(OCoLC)ocn995767577
000796526 035__ $$aSP(OCoLC)995767577$$z(OCoLC)994882836$$z(OCoLC)996402146$$z(OCoLC)999537173
000796526 040__ $$aYDX$$beng$$cYDX$$dN$T$$dEBLCP$$dGW5XE$$dN$T$$dUAB
000796526 049__ $$aISEA
000796526 050_4 $$aQB820
000796526 050_4 $$aQC1-75
000796526 08204 $$a523.2/4$$223
000796526 08204 $$a530
000796526 1001_ $$aChadney, Joshua.
000796526 24510 $$aModelling the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars /$$cJoshua Chadney.
000796526 260__ $$aCham :$$bSpringer,$$c2017.
000796526 300__ $$a1 online resource.
000796526 336__ $$atext$$btxt$$2rdacontent
000796526 337__ $$acomputer$$bc$$2rdamedia
000796526 338__ $$aonline resource$$bcr$$2rdacarrier
000796526 4901_ $$aSpringer theses
000796526 500__ $$a"Doctoral thesis accepted by Imperial College London, London, UK."
000796526 504__ $$aIncludes bibliographical references and index.
000796526 5058_ $$aSupervisors' Foreword; Preface; Acknowledgements; Contents; 1 Introduction; 1.1 Overview; 1.2 Host Stars; 1.2.1 Solar Magnetic Activity; 1.2.2 Flares; 1.2.3 Sun in Time; 1.2.4 Stellar Variability; 1.3 Planetary Upper Atmospheres; 1.3.1 Solar System Giant Planet Ionospheres: The Case of Saturn; 1.3.2 Ionospheres in Exoplanetary Systems; References; 2 Solar and Stellar X-Ray and UV Radiation; 2.1 Instrumentation for Solar and Stellar XUV Observations; 2.1.1 TIMED/SEE; 2.1.2 SORCE/XPS; 2.1.3 SDO/EVE; 2.2 Evolution of Solar Irradiance Over Different Timescales; 2.2.1 Methods
000796526 5058_ $$a2.2.2 Solar Cycle Variability2.2.3 Rotational Variability; 2.2.4 Flares; 2.2.5 XUV Flux Bands; 2.3 Stellar XUV Irradiance; 2.3.1 Absorption in the Inter-stellar Medium (ISM); 2.3.2 Coronal Model; 2.3.3 Testing the Synthetic Spectra; 2.3.4 Scaling of the Solar Spectrum; References; 3 Thermosphere; 3.1 Thermospheric Model; 3.1.1 Fluid Equations; 3.1.2 Lower Boundary; 3.1.3 Upper Boundary; 3.1.4 Photochemistry; 3.1.5 Model Runs; 3.2 Planets Orbiting Solar-Type Stars; 3.3 Planets Orbiting Other Low-Mass Stars; 3.3.1 Escape Regimes; 3.3.2 Validation of Synthetic Spectra
000796526 5058_ $$a3.3.3 Highly Enhanced Stellar X-Ray Irradiance3.4 Using Scaled Solar Spectra to Estimate Stellar XUV Emissions; 3.5 Mass Loss Rates; 3.6 Conclusion; References; 4 Ionosphere; 4.1 Ionospheric Model; 4.1.1 Ionisation Mechanisms and Theory; 4.1.2 Fluid Equations; 4.1.3 Chemical Reactions; 4.1.4 Photo-Absorption and Photo-Ionisation Cross-Sections; 4.1.5 Boundary Conditions; 4.1.6 Model Validation for the Case of Saturn; 4.2 High Resolution H2 Photo-Absorption Cross-Section; 4.3 Ionisation in Planetary Atmospheres; 4.3.1 Planets Orbiting at 1 AU from Solar-Type Stars
000796526 5058_ $$a4.3.2 Planets Orbiting Other Low-Mass Stars at 1 AU4.3.3 Using Scaled Solar Spectra; 4.3.4 Variation with Orbital Distance; 4.3.5 Flares; 4.4 Conclusion; References; 5Conclusions and FutureWork; References; Appendix A Neutral Densities; B Ion Densities from the Thermospheric Model; Index
000796526 506__ $$aAccess limited to authorized users.
000796526 588__ $$aDescription based on print version record.
000796526 650_0 $$aExtrasolar planets$$xAtmospheres$$xSimulation methods.
000796526 77608 $$iPrint version:$$z9783319633503$$z3319633503$$w(OCoLC)992747949
000796526 830_0 $$aSpringer theses.
000796526 852__ $$bebk
000796526 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-319-63351-0$$zOnline Access$$91397441.1
000796526 909CO $$ooai:library.usi.edu:796526$$pGLOBAL_SET
000796526 980__ $$aEBOOK
000796526 980__ $$aBIB
000796526 982__ $$aEbook
000796526 983__ $$aOnline
000796526 994__ $$a92$$bISE