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Thematische Bibliographien / Earths atmosphere / Bücher

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Bücher zum Thema „Earths atmosphere“

Autor: Grafiati

Veröffentlicht am 18. Mai 2024

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1

Reilly, Carmel. Earth's atmosphere. New York: Marshall Cavendish Benchmark, 2012.

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2

Borisovich, Ronov Aleksandr, und I͡A︡nshin Aleksandr Leonidovich 1911-, Hrsg. History of the Earth's atmosphere. Berlin: Springer-Verlag, 1987.

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3

B, DeMore William, Hrsg. Photochemistry of planetary atmospheres. New York: Oxford University Press, 1999.

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4

Kahn, Ralph. Comparative planetology and the atmosphere of Earth: A report to the Solar System Exploration Division, National Aeronautics and Space Administration. Pasadena, Calif: Jet Propulsion Laboratory, California Institute of Technology, 1989.

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5

David, Brodie, Nuffield Modular Sciences Project und Nuffield-Chelsea Curriculum Trust, Hrsg. Earth and atmosphere. Harlow: Published for the Nuffield-ChelseaCurriculum Trust by Longman, 1993.

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6

Syun-Ichi, Akasofu, und Kamide Y, Hrsg. The Solar wind and the earth. Tokyo, Japan: Terra Scientific Pub. Co., 1987.

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7

L, Grose William, COSPAR. Interdisciplinary Scientific Commission A. Topical Meeting, COSPAR. Interdisciplinary Scientific Commission C. Topical Meeting, COSPAR Plenary Meeting und COSPAR, Hrsg. The earth's middle atmosphere. Oxford: Published for the Committee on Space Research by Pergamon Press, 1994.

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8

Oliver, Ray. Earth, atmosphere and space. (S.l.): Thornes, 1992.

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9

L, Erukhimova Tatiana, Hrsg. Atmospheric thermodynamics: Elementary physics and chemistry. Cambridge, UK: Cambridge University Press, 2009.

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10

Wayne, Richard P. Chemistry of atmospheres: An introduction to the chemistry of the atmospheres of Earth, the planets, and their satellites. 2. Aufl. Oxford [Oxfordshire]: Oxford University Press, 1985.

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11

Chemistry of atmospheres: An introduction to the chemistry of the atmospheres of earth, the planets, and their satellites. 3. Aufl. Oxford [England]: Oxford University Press, 2000.

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12

Chemistry of atmospheres: An introduction to the chemistry of the atmospheres of Earth, the planets, and their satellites. Oxford [Oxfordshire]: Oxford University Press, 1985.

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13

Chemistry of atmospheres: An introduction to the chemistry of the atmospheres of earth, the planets, and their satellites. 2. Aufl. Oxford [England]: Clarendon Press, 1991.

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14

Robock, Alan, und Clive Oppenheimer, Hrsg. Volcanism and the Earth's Atmosphere. Washington, D. C.: American Geophysical Union, 2003. http://dx.doi.org/10.1029/gm139.

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15

Herbin, Hervé, und Philippe Dubuisson. Infrared Observation of Earth's Atmosphere. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2015. http://dx.doi.org/10.1002/9781119018490.

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16

Budyko, Michael I., Alexander B. Ronov und Alexander L. Yanshin. History of the Earth’s Atmosphere. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/978-3-642-71674-4.

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17

Council, School Examinations and Assessment. Earth and atmosphere: Science 9. London: SEAC, 1992.

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18

Eileen, Barrett, Nuffield-Chelsea Curriculum Trust und Nuffield Modular Sciences Project, Hrsg. Earth and atmosphere: Teacher's guide. Harlow: Published for the Nuffield-Chelsea Curriculum Trust by Longman, 1993.

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19

Atmospheric processes. London: Collins Educational, 1991.

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20

History Of The Earths Atmosphere. Springer, 1987.

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21

Aeronomy Of The Earths Atmosphere And Ionosphere. Springer, 2011.

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22

Chance, Kelly, und Randall V. Martin. Basic Solar and Planetary Properties. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199662104.003.0001.

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Basic properties of the Sun, the Earth and its atmosphere, other solar system atmospheres, and extrasolar planetary atmospheres are introduced here to provide background and context for the detailed study of the spectroscopy and radiative transfer of planetary atmospheres. Solar structure is described, including the solar cycle and variability, and a reference solar irradiance is presented. The Earth’s orbit, the seasons, and the ecliptic plane are introduced. The properties of hydrostatic equilibrium, albedo, and spectral reflectance are described. Earth’s atmospheric composition, including aerosols and gases, is summarized. Other atmospheres in the solar system are described and the growing field of extrasolar planets detection and characterization introduced.

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23

Calvert, Jack G., John J. Orlando, William R. Stockwell und Timothy J. Wallington. The Mechanisms of Reactions Influencing Atmospheric Ozone. Oxford University Press, 2015. http://dx.doi.org/10.1093/oso/9780190233020.001.0001.

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Ozone, an important trace component, is critical to life on Earth and to atmospheric chemistry. The presence of ozone profoundly impacts the physical structure of the atmosphere and meteorology. Ozone is also an important photolytic source for HO radicals, the driving force for most of the chemistry that occurs in the lower atmosphere, is essential to shielding biota, and is the only molecule in the atmosphere that provides protection from UV radiation in the 250-300 nm region. However, recent concerns regarding environmental issues have inspired a need for a greater understanding of ozone, and the effects that it has on the Earth's atmosphere. The Mechanisms of Reactions Influencing Atmospheric Ozone provides an overview of the chemical processes associated with the formation and loss of ozone in the atmosphere, meeting the need for a greater body of knowledge regarding atmospheric chemistry. Renowned atmospheric researcher Jack Calvert and his coauthors discuss the various chemical and physical properties of the earth's atmosphere, the ways in which ozone is formed and destroyed, and the mechanisms of various ozone chemical reactions in the different spheres of the atmosphere. The volume is rich with valuable knowledge and useful descriptions, and will appeal to environmental scientists and engineers alike. A thorough analysis of the processes related to tropospheric ozone, The Mechanisms of Reactions Influencing Atmospheric Ozone is an essential resource for those hoping to combat the continuing and future environmental problems, particularly issues that require a deeper understanding of atmospheric chemistry.

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24

Flores, Eleanor. Atmospheric Science: Understanding the Earth's Atmosphere. Syrawood Publishing House, 2021.

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25

Light, Charlie. Observing Earth: Investigating Earth's Atmosphere. Stevens Publishing LLLP, Gareth, 2020.

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26

Light, Charlie. Observing Earth: Investigating Earth's Atmosphere. Stevens Publishing LLLP, Gareth, 2020.

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27

Light, Charlie. Observing Earth: Investigating Earth's Atmosphere. Stevens Publishing LLLP, Gareth, 2020.

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28

Palmer, Paul I. The Atmosphere: A Very Short Introduction. Oxford University Press, 2017. http://dx.doi.org/10.1093/actrade/9780198722038.001.0001.

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The atmosphere is the thin, diffuse fluid that envelops the Earth’s surface. Despite its apparent fragility, the existence of this fluid is vital for human and other life on Earth. The Atmosphere: A Very Short Introduction describes the physical and chemical characteristics of different layers in the atmosphere, and shows how the atmosphere’s interactions with land, ocean, and ice affect these properties. It also looks at how movement in the atmosphere, driven by heat from the Sun, transports heat from lower latitudes to higher latitudes. Finally, it presents an overview of the types of measurements used to understand different parts of the atmosphere, and identifies future challenges in the light of climate change.

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29

Introduction to Atmospheric Chemistry. Cambridge University Press, 2000.

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30

Introduction to Atmospheric Chemistry. Cambridge University Press, 2001.

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31

Hobbs, Peter V. Introduction to Atmospheric Chemistry. Cambridge University Press, 2012.

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32

Yung, Yuk L., und William B. DeMore. Photochemistry of Planetary Atmospheres. Oxford University Press, Incorporated, 1998.

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33

Spradley, Joe, David Kenneth Elliott, Margaret Boorstein und Steven I. Dutch. Earth Science: Earth's Weather, Water and Atmosphere. Salem Press, Incorporated, 2012.

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34

James, Ph.D. Trefil (Contributor), Rita Ann, Ph.D. Calvo (Contributor) und Kenneth Ms Cutler (Contributor), Hrsg. Earth's Atmosphere (Mcdougal Littell Science: Earth Science). Houghton Mifflin School, 2006.

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35

Wolf, E. L. Solar Radiation through the Atmosphere. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198769804.003.0003.

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Maxwell’s equations describe radiated power from the Sun through space and the atmosphere to the Earth. Black-body radiation arises from matter in thermal equilibrium, as is derived in this chapter. The Stefan–Boltzmann power law is derived, and its consequences are discussed. Basics of the atmosphere are discussed, including kinetic energy arising from the condensation of water vapor to liquid water. The temperatures in the atmosphere are discussed in a layered model. The Sun’s light arrives at Earth through vacuum and the Earth’s atmosphere as electromagnetic waves described by Maxwell’s equations. In contemporary electrical engineering jargon, this is “wireless”, that connects cellphones.

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36

Shofner, Melissa Raé. Earth's Atmosphere. Rosen Publishing Group, 2018.

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37

Earth's Atmosphere. Rosen Publishing Group, 2018.

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38

Shofner, Melissa Raé. Earth's Atmosphere. Rosen Publishing Group, 2018.

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39

Earth's Atmosphere. McDougal Littell, 2005.

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40

Harman, Rebecca. Carbon-oxygen And Nitrogen Cycles (Earth's Processes). Heinemann, 2005.

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41

Vlasov, Sergey, Olga Konovalova, Irina Chudovskaya, Inna Vlasova, Natalia Kolotilova und Valery Snakin. Methane in the atmosphere, methanotrophs and development of oil and gas industry. LLC MAKS Press, 2021. http://dx.doi.org/10.29003/m1986.978-5-317-06580-5.

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Dynamics of methane content alterations in the Earth's atmosphere in the conditions of globalization is analyzed and methane emission sources are estimated. Oil and gas industry is proved to be the most important anthropogenic source of atmospheric methane growth. Natural mechanisms of methane concentration regulation in the biosphere are considered. Particular attention is paid to the process of methane absorption by methanotrophic microorganisms and peculiarities of their functioning in extreme conditions. Methodology for reducing methane technogenic inflow into the atmosphere using methanotrophs is proposed. The book is addressed to oil and gas industry employees and everyone interested in the behavior of methane in the atmosphere, especially in connection with the atmospheric pollution and natural degradation of pollutants.

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42

Chance, Kelly, und Randall V. Martin. Spectroscopy and Radiative Transfer of Planetary Atmospheres. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199662104.001.0001.

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This book develops both spectroscopy and radiative transfer for planetary atmospheric composition in a rigorous and quantitative sense for students of atmospheric and/or planetary science. Spectroscopic field measurements including satellite remote sensing have advanced rapidly in recent years, and are being increasingly applied to provide information about planetary atmospheres. Examples include systematic observation of the atmospheric constituents that affect weather, climate, biogeochemical cycles, air quality on Earth, as well as the physics and evolution of planetary atmospheres in our solar system and beyond. Understanding atmospheric spectroscopy and radiative transfer is important throughout the disciplines of atmospheric science and planetary atmospheres to understand principles of remote sensing of atmospheric composition and the effects of atmospheric composition on climate. Atmospheric scientists need an understanding of the details, strength and weaknesses of the spectroscopic measurement sources. Those in remote sensing require an understanding of the information content of the measured spectra that are needed for the design of retrieval algorithms and for developing new instrumentation.

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43

Canfield, Donald Eugene. The Great Oxidation. Princeton University Press, 2017. http://dx.doi.org/10.23943/princeton/9780691145020.003.0008.

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This chapter deals with the “great oxidation event” (GOE), which represents a quantum shift in the oxygen content of the atmosphere. It suggests that the GOE represents the evolution of cyanobacteria. According to the geologic record, the oxygen content of Earth's atmosphere increased dramatically around 2.3 billion years ago. Since cyanobacteria likely evolved much earlier, it does not appear that a well-oxygenated atmosphere is a necessary or immediate consequence of the activities of oxygen-producing organisms. Atmospheric chemistry is a slave to the dynamics of the mantle, as the interior and exterior of the planet are connected in a profound way. Indeed, it took half of Earth's history for the mantle to quiet to point where oxygen could accumulate. This, however, represented a watershed, a tipping point if you will, where the chemistry of Earth's surface was forever altered.

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44

Grose, W. L., A. Ghazi und M. A. Geller. Earth's Middle Atmosphere. Elsevier Science & Technology Books, 2016.

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45

The Earth’s Atmosphere. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-78427-2.

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46

Saha, Kshudiram. The Earth's Atmosphere. Springer, 2009.

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47

Pedersen, Traci Steckel. The Earth's Atmosphere. Perfection Learning, 2007.

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48

AVP. Earth and Atmosphere. Cascade Marketing Intl Inc, 1996.

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49

BOOKS, Editors of TIME-LIFE, und Oliver E. Allen. Atmosphere (Planet Earth). Time Life Education, 1985.

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50

Goody, R. M., und Y. L. Yung. Atmospheric Radiation. Oxford University Press, 1989. http://dx.doi.org/10.1093/oso/9780195051346.001.0001.

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A complete revision of Goody's classic 1964 work, this volume offers a systematic discussion of atmospheric radiation processes that today are at the center of worldwide study and concern. It deals with the ways in which incident solar radiation is transformed into scattered and thermal radiation, and the thermodynamic consequences for the Earth's gaseous envelope, identifying aspects of the interaction between radiation and atmospheric motions as the central theme for atmospheric radiation studies. As a complete treatment of physical and mathematical foundations, the text assumes no prior knowledge of atmospheric physics. The theoretical discussion is systematic, and can therefore be applied with minor extension to any planetary atmosphere.

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