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Titlebook: Aeronomy of Mars; S. A. Haider Book 2023 Springer Nature Singapore Pte Ltd. 2023 Mars Upper Ionosphere.Modeling the Martian atmosphere.Ion

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发表于 2025-3-21 19:15:52 | 显示全部楼层 |阅读模式
期刊全称Aeronomy of Mars
影响因子2023S. A. Haider
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发行地址Is the first-ever one on the aeronomy of Mars and reviewing the results from all Mars missions.Highlights various models on the aeronomy of Mars and complements them with experimental data.Aims for st
学科分类Astrophysics and Space Science Library
图书封面Titlebook: Aeronomy of Mars;  S. A. Haider Book 2023 Springer Nature Singapore Pte Ltd. 2023 Mars Upper Ionosphere.Modeling the Martian atmosphere.Ion
影响因子.“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”..
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发表于 2025-3-21 20:54:17 | 显示全部楼层
Foundation of Ionospheric Theory,polar diffusion, eddy diffusion and thermal energy balance. Using these equations the ion densities, electron densities and temperature structures can be studied in the lower and upper ionosphere of Mars.
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Magnetic Field of Mars, .; Acuña et al. Science 279:1676–1680, .). Later observations were carried out by Mars 2 to 7 and Phobos − 2 in 1970 and 1989 respectively (Riedler et al. Planet Space Sci. 39:75–81, .; Slavin et al. J. Geophys. Res. Space Phys. 96:11235–11241, .; Möhlmann et al. Adv Space Res 12:221–229, .). These
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Upper Atmosphere of Mars, is primarily composed of CO. (95%), N. (2.8%) and Ar (2%) (Villanueva et al., Icarus 223:11–27, .); (Franz et al., Planet Space Sci. 138:44–54, .). It also contains trace gases like H.O, O, CO, H. and noble gases (Villanueva et al., Icarus 223:11–27, .); (Franz et al., Planet Space Sci. 138:44–54,
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