Gotowe bibliografie tematyczne / Atmosphere

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji
  6. Raporty organizacyjne

Gotowa bibliografia na temat „Atmosphere”

Autor: Grafiati
Data publikacji: 4 czerwca 2021
Data aktualizacji: 25 lipca 2025

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Artykuły w czasopismach na temat "Atmosphere"

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Sergeev, Denis E., Nathan J. Mayne, Thomas Bendall, et al. "Simulations of idealised 3D atmospheric flows on terrestrial planets using LFRic-Atmosphere." Geoscientific Model Development 16, no. 19 (2023): 5601–26. http://dx.doi.org/10.5194/gmd-16-5601-2023.

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Abstract. We demonstrate that LFRic-Atmosphere, a model built using the Met Office's GungHo dynamical core, is able to reproduce idealised large-scale atmospheric circulation patterns specified by several widely used benchmark recipes. This is motivated by the rapid rate of exoplanet discovery and the ever-growing need for numerical modelling and characterisation of their atmospheres. Here we present LFRic-Atmosphere's results for the idealised tests imitating circulation regimes commonly used in the exoplanet modelling community. The benchmarks include three analytic forcing cases: the standa
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Ragossnig, Florian, Alexander Stökl, Ernst Dorfi, Colin P. Johnstone, Daniel Steiner, and Manuel Güdel. "Interaction of infalling solid bodies with primordial atmospheres of disk-embedded planets." Astronomy & Astrophysics 618 (October 2018): A19. http://dx.doi.org/10.1051/0004-6361/201832681.

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Context. Planets that form early enough to be embedded in the circumstellar gas disk accumulate thick atmospheres of nebular gas. Models of these atmospheres need to specify the surface luminosity (i.e. energy loss rate) of the planet. This luminosity is usually associated with a continuous inflow of solid bodies, where the gravitational energy released from these bodies is the source of energy. However, if these bodies release energy in the atmosphere instead of at the surface, this assumption might not be justified. Aims. Our aim is to explore the interactions of infalling planetesimals with
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Chouqar, J., Z. Benkhaldoun, A. Jabiri, J. Lustig-Yaeger, A. Soubkiou, and A. Szentgyorgyi. "Properties of sub-Neptune atmospheres: TOI-270 system." Monthly Notices of the Royal Astronomical Society 495, no. 1 (2020): 962–70. http://dx.doi.org/10.1093/mnras/staa1198.

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ABSTRACT We investigate the potential for the James Webb Space Telescope (JWST) to detect and characterize the atmospheres of the sub-Neptunian exoplanets in the TOI-270 system. Sub-Neptunes are considered more likely to be water worlds than gas dwarfs. We model their atmospheres using three atmospheric compositions – two examples of hydrogen-dominated atmospheres and a water-dominated atmosphere. We then simulate the infrared transmission spectra of these atmospheres for JWST instrument modes optimized for transit observation of exoplanet atmospheres: NIRISS, NIRSpec, and MIRI. We then predic
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Sysoeva, Yu V. "Проблема атмосферы у Г. Беме и ее отношение к цифровой культуре". Studia Culturae, № 56 (2 листопада 2023): 120. http://dx.doi.org/10.31312/2310-1245-2023-56-120-143.

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This article is devoted to a relatively new aesthetic concept, the concept of atmosphere. In the second half of the 20th century, due to the overcoming of the understanding of the aesthetic as a field of art and the emergence of the tendency to appeal to sensual experience, the idea that aesthetic perception and aesthetic experience are possible not only in the context of art events, but also in the space of everyday life is becoming increasingly relevant. The aesthetics of atmosphere arises from the aesthetics of everyday life. The first to declare the concept of atmosphere as a separate aest
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Seager, Sara. "Exoplanet atmospheres: A theoretical outlook." Proceedings of the International Astronomical Union 6, S276 (2010): 198–207. http://dx.doi.org/10.1017/s1743921311020187.

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AbstractWith over two dozen exoplanet atmospheres observed today, the field of exoplanet atmospheres is solidly established. The highlights of exoplanet atmosphere studies include: detection of molecular spectral features; constraints on atmospheric vertical temperature structure; detection of day-night temperature gradients; and a new numerical approach to atmosphere temperature and abundance retrieval. As hot Jupiter observations and interpretation are maturing, the next frontier is super Earth atmospheres. Theoretical models of super Earth atmospheres are moving forward with observational h
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Miller-Ricci, Eliza, Sara Seager, and Dimitar Sasselov. "The Atmospheres of Extrasolar Super-Earths." Proceedings of the International Astronomical Union 4, S253 (2008): 263–71. http://dx.doi.org/10.1017/s1743921308026483.

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AbstractExtrasolar super-Earths (1-10 M⊕) are likely to exist with a wide range of atmospheres. While a number of these planets have already been discovered through radial velocities and microlensing, it will be the discovery of the firsttransitingsuper-Earths that will open the door to a variety of follow-up observations aimed at characterizing their atmospheres. Super-Earths may fill a large range of parameter space in terms of their atmospheric composition and mass. Specifically, some of these planets may have high enough surface gravities to be able to retain large hydrogen-rich atmosphser
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Wachiraphan, Patcharapol, Zachory K. Berta-Thompson, Hannah Diamond-Lowe, et al. "The Thermal Emission Spectrum of the Nearby Rocky Exoplanet LTT 1445A b from JWST MIRI/LRS." Astronomical Journal 169, no. 6 (2025): 311. https://doi.org/10.3847/1538-3881/adc990.

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Abstract The nearby transiting rocky exoplanet LTT 1445A b presents an ideal target for studying atmospheric retention in terrestrial planets orbiting M dwarfs. It is cooler than many rocky exoplanets yet tested for atmospheres, receiving a bolometric instellation similar to Mercury’s. Previous transmission spectroscopy ruled out a light H/He-dominated atmosphere but could not distinguish between a bare-rock, a high-MMW, nor a cloudy atmosphere. We present new secondary eclipse observations using JWST’s MIRI/LRS, covering the 5–12 μm range. From these observations, we detect a broadband second
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Bisikalo, Dmitri, Valery Shematovich, and Benoit Hubert. "The Kinetic Monte Carlo Model of the Auroral Electron Precipitation into N2-O2 Planetary Atmospheres." Universe 8, no. 8 (2022): 437. http://dx.doi.org/10.3390/universe8080437.

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Auroral events are the prominent manifestation of solar/stellar forcing on planetary atmospheres. They are closely related to the energy deposition by and evolution of planetary atmospheres, and their observations are widely used to analyze the composition, structure, and chemistry of the atmosphere under study, as well as energy fluxes of the precipitating particles that affect the atmosphere. A numerical kinetic Monte Carlo model had been developed, allowing us to study the processes of precipitation of high-energy auroral electrons into the N2-O2 atmospheres of the rocky planets in the Sola
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Kurosaki, Kenji, and Shu-ichiro Inutsuka. "Giant Impact Events for Protoplanets: Energetics of Atmospheric Erosion by Head-on Collision." Astrophysical Journal 954, no. 2 (2023): 196. http://dx.doi.org/10.3847/1538-4357/ace9ba.

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Abstract Numerous exoplanets with masses ranging from Earth to Neptune and radii larger than Earth have been found through observations. These planets possess atmospheres that range in mass fractions from 1% to 30%, reflecting the diversity of atmospheric mass fractions. Such diversities are supposed to be caused by differences in the formation processes or evolution. Here, we consider head-on giant impacts onto planets causing atmosphere losses in the later stage of their formation. We perform smoothed particle hydrodynamic simulations to study the impact-induced atmosphere loss of young supe
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Johnstone, Colin P. "The Influences of Stellar Activity on Planetary Atmospheres." Proceedings of the International Astronomical Union 12, S328 (2016): 168–79. http://dx.doi.org/10.1017/s1743921317003775.

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AbstractOn evolutionary timescales, the atmospheres of planets evolve due to interactions with the planet's surface and with the planet's host star. Stellar X-ray and EUV (=’XUV’) radiation is absorbed high in the atmosphere, driving photochemistry, heating the gas, and causing atmospheric expansion and mass loss. Atmospheres can interact strongly with the stellar winds, leading to additional mass loss. In this review, I summarise some of the ways in which stellar output can influence the atmospheres of planets. I will discuss the importance of simultaneously understanding the evolution of the
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Rozprawy doktorskie na temat "Atmosphere"

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McElroy, Kenneth L. "The atmospheric emission method of calculating the neutral atmosphere and changed particle densities in the upper atmosphere." Thesis, Monterey, California. Naval Postgraduate School, 1992. http://hdl.handle.net/10945/23548.

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Martello, Robert 1968. "Land atmosphere interaction and atmospheric mixed layer height evolution." Thesis, Massachusetts Institute of Technology, 1996. http://hdl.handle.net/1721.1/38774.

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Erculiani, Marco. "Atmosphere in a test tube: laboratory investigations about exoplanet atmospheres." Doctoral thesis, Università degli studi di Padova, 2015. http://hdl.handle.net/11577/3424370.

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The aim of this thesis is to understand if cyanobacteria, grown on an Earth-like planet orbiting around the habitable zone of an M star can survive and use the light coming from the star in a fruitful way, in particular analyzing their gaseous by-products. The organisms chosen usually don't have photopigments capable to photosynthesize the NIR part of the radiation, but can modify their photosynthetic apparatus in order to adapt to different light conditions if exposed in NIR light conditions, producing chlorophyll d and f. The two bacteria highlighted for our purpose are Chlorogloeopsis frits
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Tice, Dane Steven. "Ground-based near-infrared remote sounding of ice giant clouds and methane." Thesis, University of Oxford, 2014. http://ora.ox.ac.uk/objects/uuid:4f09f270-a25c-4d36-96d3-13070a594eaa.

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The ice giants, Uranus and Neptune, are the two outermost planets in our solar system. With only one satellite flyby each in the late 1980’s, the ice giants are arguably the least understood of the planets orbiting the Sun. A better understanding of these planets’ atmospheres will not only help satisfy the natural scientific curiosity we have about these distant spheres of gas, but also might provide insight into the dynamics and meteorology of our own planet’s atmosphere. Two new ground-based, near-infrared datasets of the ice giants are studied. Both datasets provide data in a portion of the
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Franks, Stewart William. "The representation of land surface - atmosphere fluxes for atmospheric modelling." Thesis, Lancaster University, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.387430.

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Rose, Kathleen A. "Environment "atmosphere" /." Online version of thesis, 1989. http://hdl.handle.net/1850/11084.

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Steiner, Allison L. "The influence of atmospheric chemistry and climate on atmosphere-biosphere interactions." Diss., Georgia Institute of Technology, 2003. http://hdl.handle.net/1853/25751.

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Eichelberger, Scott James. "The effects of meridional heating gradients on the atmospheric general circulation and its variability /." Thesis, Connect to this title online; UW restricted, 2005. http://hdl.handle.net/1773/10029.

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Geißler, Christoph, and Ch Jacobi. "Forcing of the Quarterdiurnal Tide." Universität Leipzig, 2018. https://ul.qucosa.de/id/qucosa%3A31792.

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Ensemble calculations for the period from 2000 to 2010 were carried out with the middle and upper atmosphere model (MUAM), and an analysis of the quarterdiurnal tide is performed. The global temporal and latitudinal distributions of the quarterdiurnal tide are modeled with MUAM, and their forcing mechanisms are examined. The quarterdiurnal tides show a similar distribution over the year in the northern and southern hemisphere, with maxima of the amplitude in late winter and spring as well as in autumn. In the latitude-height distribution is also shown that the largest amplitudes of the quarter
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Sefcik, Lesley T. "Biophere-atmosphere interactions Northern hardwood seedling responses to anthropogenic atmospheric resource alteration." Saarbrücken VDM Verlag Dr. Müller, 2001. http://d-nb.info/988972131/04.

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Książki na temat "Atmosphere"

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Schaefer, Vincent J. The atmosphere. Houghton Mifflin, 1990.

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Rees, M. H. Physics and chemistry of the upper atmosphere. Cambridge University Press, 1989.

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Desonie, Dana. Atmosphere. Chelsea House, 2007.

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Lister, Anne. Atmosphere. Program Services, Vancouver School Board, 1990.

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Copyright Paperback Collection (Library of Congress), ed. Atmosphere. Leisure Books, 2002.

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B, Singh H., ed. Composition, chemistry, and climate of the atmosphere. Van Nostrand Reinhold, 1995.

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United States. National Aeronautics and Space Administration, ed. Upper atmosphere research satellite: Remote atmospheric sensors. National Aeronautics and Space Administration, 1989.

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F, Keeling Ralph, ed. The atmosphere. Elsevier, 2006.

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Georgii, H. W. Von der Physik zur Chemie der freien Atmosphäre. F. Steiner, 1995.

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Groves, Gerald Vann. A global reference atmosphere from 18 to 80 km. Atmospheric Sciences Division, Air Force Geophysics Laboratory, 1985.

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Części książek na temat "Atmosphere"

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Gooch, Jan W. "Atmosphere (Standard Atmosphere)." In Encyclopedic Dictionary of Polymers. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-6247-8_879.

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Griffero, Tonino. "Atmosphere." In Lecture Notes in Morphogenesis. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-51324-5_7.

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Gambaro, Andrea, Elena Gregoris, and Carlo Barbante. "Atmosphere." In Environmental Analysis by Electrochemical Sensors and Biosensors. Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4939-0676-5_4.

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Tawa, Michael. "Atmosphere." In Atmosphere, Architecture, Cinema. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-13964-2_5.

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Sadraey, Mohammad H. "Atmosphere." In Aircraft Performance. CRC Press, 2017. http://dx.doi.org/10.1201/9781315366913-1.

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Weik, Martin H. "atmosphere." In Computer Science and Communications Dictionary. Springer US, 2000. http://dx.doi.org/10.1007/1-4020-0613-6_951.

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Añel, Juan A. "Atmosphere." In The Environment in Galicia: A Book of Images. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-33114-5_1.

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Sadraey, Mohammad H. "Atmosphere." In Aircraft Performance, 2nd ed. CRC Press, 2023. http://dx.doi.org/10.1201/9781003279068-1.

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Schmieder, Robert William. "Atmosphere." In Heard Island. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-20343-5_29.

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Pleter, Octavian Thor. "Atmosphere." In Air Navigation. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-52994-8_3.

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Streszczenia konferencji na temat "Atmosphere"

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Carpio, J. J., J. Reyes, G. Hernández-Duque, and L. Martínez. "Determination of Atmospheric Corrosivity in the South East Gulf of Mexico." In CORROSION 1995. NACE International, 1995. https://doi.org/10.5006/c1995-95238.

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Abstract Atmospheric corrosion in the south east region of Gulf of Mexico can be intense and affect to a great extent the coastal economy, as the industrial installations and equipments are attacked sinergistically by natural and anthropogenic atmospheric pollutants. The corrosivity of atmospheres in this region is being studied and characterized by means of the ISO 9223: 1992 standard methodology. This study presents the preliminary results obtained at five different sites in the Gulf. Iron, copper, zinc and aluminium plates are exposed in metallic panels and the deposition rates of chlorides
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Bratcher, Damian. "Protective Atmospheres, Measurement Technologies, and Troubleshooting Tools." In HT 2013, edited by B. Lynn Ferguson. ASM International, 2013. https://doi.org/10.31399/asm.cp.ht2013p0213.

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Abstract Furnace atmospheres are critical to meeting metallurgical specifications defined by control processes. The makeup of a furnace's atmosphere in the heat treating process varies based upon the application. This session will cover the different types of atmospheres, the sensors used to measure the atmosphere, and troubleshooting procedures for validation of the environment.
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Bernard, Benjamin T. "Ferritic Nitrocarburizing Processes and Applications." In HT 2013, edited by B. Lynn Ferguson. ASM International, 2013. https://doi.org/10.31399/asm.cp.ht2013p0170.

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Abstract Ferritic Nitrocarburizing and nitriding processes are available in various atmosphere blends and a myriad of equipment designs. Atmosphere choices can dictate process capabilities. Equipment design should be reviewed to select the proper choice for the part application. Atmosphere control, nitriding potential calculations, as well as selecting atmospheres and proper heat treat equipment are included.
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Madani, Mahmoud, and Richard D. Granata. "Study of Akaganeite in Weathering Steel Corrosion Products and Distance from Ocean in South Florida." In CORROSION 2018. NACE International, 2018. https://doi.org/10.5006/c2018-11337.

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Abstract The corrosion of mild steel in chloride-rich atmospheres is a highly topical issue for industry and departments of transportation. The formation of the oxyhydroxide akaganeite (β-FeOOH) in this type of atmosphere is associated with a notable acceleration of the steel corrosion process. The scientific literature contains many references to outdoor marine atmospheric tests, but has not yet clarified some issues regarding akaganeite, such as, the environmental conditions for its formation. Research has been performed at thirty atmospheric corrosion stations located at south Florida withi
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Hartwig, Charles, and John W. Gottschalk. "Flexible Controlled Atmosphere Hardening Processes Utilizing Atmosphere Furnaces and Salt Quenching Systems." In HT 2013, edited by B. Lynn Ferguson. ASM International, 2013. https://doi.org/10.31399/asm.cp.ht2013p0249.

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Abstract This presentation will discuss a flexible atmosphere heat treating system employing salt quench systems that are considerably faster, than existing technology utilizing internal quench systems. Topics include: improved temperature control, temperature uniformity/uniformity of the austenitizing process; improved automation and reliability of material handling transfers from the austenitizing furnace to the quench system; and increased flexibility, with regard to the quench system, to allow for the widest range of processes to be run in the system.
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Nakagawa, Kiyokazu, and Teiichi Isozaki. "Fireside Corrosion in Reducing Waste Incineration Environments." In CORROSION 1994. NACE International, 1994. https://doi.org/10.5006/c1994-94177.

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Abstract The corrosion behavior of a carbon steel covered with synthetic ashes and an actual ash has been investigated under reducing and oxidizing atmospheres. It has become clear that HCl content has a great influence on the corrosion rate of the carbon steel covered with NaCl-KCl and NaCl-KCl-Na2SO4-K2SO4 in the reducing atmosphere. When the HCl content in the reducing gas was 0.2%, a severe corrosion attack was observed at 350°C and 400°C. This corrosion is considered to be due to NaCl-KCl-FeCl2 hot corrosion. In the oxidizing atmosphere the corrosion was slight at all temperatures tested.
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Lifka, B. W. "Corrosion Resistance of Aluminum Alloy Plate in Rural, Industrial, and Seacoast Atmospheres." In CORROSION 1987. NACE International, 1987. https://doi.org/10.5006/c1987-87420.

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Abstract Stress corrosion and exfoliation corrosion test specimens from aluminum alloy plates have completed five years of a scheduled 20 year exposure program in rural atmosphere at Alcoa Center, PA, industrial atmosphere at Los Angeles, CA, and seacoast atmosphere at Point Judith, RI. The materials being evaluated are 19 mm and 64 mm thick plates of the following nine alloys and tempers: 2024-T351 and T851, 5456-H116, 6061- T651, 7050-T7651 and T7451 and 7075- T651, T7651, and T7351. Test data are presented for 6 months, and 1, 2, and 5 years of exposure. In general, the effects of corrosion
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Oakes, Jim. "Understanding Furnace Atmosphere Composition for Neutral and Gas Carburizing Applications." In HT 2015. ASM International, 2015. http://dx.doi.org/10.31399/asm.cp.ht2015p0229.

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Abstract Studying the gas composition of an atmosphere furnace reveals many parameters that can be used to predict metallurgical results of parts being processed. Today’s heat treaters strive for process consistency in order to eliminate variability, rework, and (in the worst case) scrap. In atmosphere heat treating, understanding control parameters and atmosphere composition provides critical insight into expected results. In this presentation, the audience will have the opportunity to observe gas compositions that would typically be found in carbon-neutral or carbon-rich atmospheres; they wi
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Strow, L. Larrabee. "A Signal-Processing Approach for the Retrieval of Global Tropospheric CO Using the Atmospheric Infrared Sounder (AIRS)." In Optical Remote Sensing of the Atmosphere. Optica Publishing Group, 1993. http://dx.doi.org/10.1364/orsa.1993.the.9.

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One goal of the Earth Observing Systems (EOS) is to measure concentrations of key atmospheric gases on a global scale in order to understand biogeochemical cycles in both the natural, unpolluted atmosphere, and in regions where anthropogenic activities have perturbed concentrations of gas-phase species. A particular concern in tropospheric chemistry is that increasing levels of carbon monoxide (CO) may lead to a decrease in atmospheric hydroxyl (OH) which would reduce the atmosphere's ability to scavenge other trace gases.
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Sadot, D. "Thermal imaging through the atmosphere: atmospheric MTF." In 16th Congress of the International Commission for Optics: Optics as a Key to High Technology. SPIE, 1993. http://dx.doi.org/10.1117/12.2308551.

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Raporty organizacyjne na temat "Atmosphere"

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Davis, K. J., S. J. Richardson, and N. L. Miles. Regional Ecosystem-Atmosphere CO2 Exchange Via Atmospheric Budgets. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/900475.

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Stanley, Rachel H. R., Thomas Thomas, Yuan Gao, et al. US SOLAS Science Report. Woods Hole Oceanographic Institution, 2021. http://dx.doi.org/10.1575/1912/27821.

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The Surface Ocean – Lower Atmosphere Study (SOLAS) (http://www.solas-int.org/) is an international research initiative focused on understanding the key biogeochemical-physical interactions and feedbacks between the ocean and atmosphere that are critical elements of climate and global biogeochemical cycles. Following the release of the SOLAS Decadal Science Plan (2015-2025) (Brévière et al., 2016), the Ocean-Atmosphere Interaction Committee (OAIC) was formed as a subcommittee of the Ocean Carbon and Biogeochemistry (OCB) Scientific Steering Committee to coordinate US SOLAS efforts and activitie
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Leacock, John. Neutron Propagation in Atmosphere. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1159564.

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Dorsey, Kathryn, and Daniel Feldman. Surface Atmosphere Integrated Field Laboratory. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1669356.

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Marland, G. (Chemistry of the global atmosphere). Office of Scientific and Technical Information (OSTI), 1990. http://dx.doi.org/10.2172/6539398.

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Kayser, David C., William T. Chater, Charles K. Howey, and James B. Pranke. The Upper Atmosphere Composition Spectrometer. Defense Technical Information Center, 1986. http://dx.doi.org/10.21236/ada175788.

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Ostashev, V. E., and G. H. Goedecke. Acoustic Tomography of the Atmosphere. Defense Technical Information Center, 2007. http://dx.doi.org/10.21236/ada470885.

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Rogers, David P. Coupled Ocean-Atmosphere Interaction and the Development of the Marine Atmospheric Boundary Layer. Defense Technical Information Center, 1997. http://dx.doi.org/10.21236/ada330047.

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Rogers, David P. Coupled Ocean-Atmosphere Interaction and the Development of the Marine Atmospheric Boundary Layer. Defense Technical Information Center, 2000. http://dx.doi.org/10.21236/ada383683.

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Douglas, Thomas, and Joel Blum. Mercury isotopes reveal atmospheric gaseous mercury deposition directly to the Arctic coastal snowpack. Engineer Research and Development Center (U.S.), 2021. http://dx.doi.org/10.21079/11681/41046.

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Streszczenie:
Springtime atmospheric mercury depletion events (AMDEs) lead to snow with elevated mercury concentrations (>200 ng Hg/L) in the Arctic and Antarctic. During AMDEs gaseous elemental mercury (GEM) is photochemically oxidized by halogens to reactive gaseous mercury which is deposited to the snowpack. This reactive mercury is either photochemically reduced back to GEM and reemitted to the atmosphere or remains in the snowpack until spring snowmelt. GEM is also deposited to the snowpack and tundra vegetation by reactive surface uptake (dry deposition) from the atmosphere. There is little consens
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