04299nam 22007215 450 991074115660332120251009071939.0981-9931-38-X10.1007/978-981-99-3138-5(MiAaPQ)EBC30706860(CKB)27994393400041(Au-PeEL)EBL30706860(DE-He213)978-981-99-3138-5(PPN)272260541(EXLCZ)992799439340004120230817d2023 u| 0engurcnu||||||||txtrdacontentcrdamediacrrdacarrierAeronomy of Mars /by S. A. Haider1st ed. 2023.Singapore :Springer Nature Singapore :Imprint: Springer,2023.1 online resource (259 pages)Astrophysics and Space Science Library,2214-7985 ;4699789819931378 Introduction -- Foundation of Ionospheric Theory -- Instruments for Ionospheric Measurements on Mars -- Exploration to Mars Atmosphere -- Thermal Structure of Mars Atmosphere -- Magnetic Field of Mars -- Upper Atmosphere of Mars -- Atmospheric Escape from Mars -- Upper Ionosphere of Mars -- Heating of the Upper Ionosphere of Mars -- Models of the Martian ionosphere -- Solar Flux for Ionospheric Modeling of Mars -- Cross Sections for Ionospheric Modeling of Mars -- Ionization Sources of Upper Ionosphere of Mars -- Mars Upper Ionospheric Disturbances -- Upper Ionosphere of Mars during Low, Medium and High Solar Activity -- Airglow on Mars -- Middle Ionosphere of Mars -- Gravity Waves in the Middle Atmosphere of Mars -- Lower Atmosphere of Mars -- Trace Gases of Mars Atmosphere -- Seasonal Variability of Atmospheric Gases -- Infrared Thermal Emissions from Mars Atmosphere -- Lower Ionosphere of Mars -- Conductivity -- Dust Storm in the Lower Atmosphere of Mars -- Summary and Conclusions -- References.“Mangalyaan was launched on November 5, 2013, to Mars by Indian Space Research Organization (ISRO). On October 2, 2022, ISRO declared that Mangalyaan had lost communications with Earth. Mars Color Camera (MCC) on-board Mangalyaan has taken thousands pictures of Mars. A full disk of Mars image observed by Viking is shown on the cover page of this book. Mars is covered by the dust as observed by Mangalyaan (from Arya et al., 2015). This book presents the atmospheric and ionospheric results obtained from all missions to Mars. It also covers various atmospheric and ionospheric models of Mars. Broadly speaking, the planet’s atmosphere can be divided into two regions: lower and upper. These two regions can be coupled due to the propagation of energy from the lower to the upper atmosphere. The first-ever book on the aeronomy of Mars, this work is intended to help students and researchers familiarize themselves with the field of aeronomy. In addition, it helps planetary probe designers, engineers, and other users in the scientific community, e.g., planetary geologists and geophysicists”.Astrophysics and Space Science Library,2214-7985 ;469Solar systemAstronomyObservationsPhysical geographyMathematical physicsPlanetary sciencePlasma (Ionized gases)Space PhysicsAstronomy, Observations and TechniquesEarth System SciencesTheoretical, Mathematical and Computational PhysicsPlanetary SciencePlasma PhysicsSolar system.AstronomyPhysical geography.Mathematical physics.Planetary science.Plasma (Ionized gases)Space Physics.Astronomy, Observations and Techniques.Earth System Sciences.Theoretical, Mathematical and Computational Physics.Planetary Science.Plasma Physics.551.5099923Haider S. A1424919MiAaPQMiAaPQMiAaPQBOOK9910741156603321Aeronomy of Mars3554557UNINA