Relevant bibliographies by topics / Atmospheric

Academic literature on the topic 'Atmospheric'

Author: Grafiati
Published: 4 June 2021
Last updated: 30 July 2024

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Journal articles on the topic "Atmospheric"

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Habib, Namrah, and Raymond T. Pierrehumbert. "Modeling Noncondensing Compositional Convection for Applications to Super-Earth and Sub-Neptune Atmospheres." Astrophysical Journal 961, no. 1 (January 1, 2024): 35. http://dx.doi.org/10.3847/1538-4357/ad04e2.

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Abstract Compositional convection is atmospheric mixing driven by density variations caused by compositional gradients. Previous studies have suggested that compositional gradients of atmospheric trace species within planetary atmospheres can impact convection and the final atmospheric temperature profile. In this work, we employ 3D convection-resolving simulations using Cloud Model 1 (CM1) to gain a fundamental understanding of how compositional variation influences convection and the final atmospheric state of exoplanet atmospheres. We perform 3D initial value problem simulations of noncondensing compositional convection for Earth-air, H2, and CO2 atmospheres. Conventionally, atmospheric convection is assumed to mix the atmosphere to a final, marginally stable state defined by a unique temperature profile. However, when there is compositional variation within an atmosphere, a continuous family of stable end states is possible, differing in the final state composition profile. Our CM1 simulations are used to determine which of the family of possible compositional end states is selected. Leveraging the results from our CM1 simulations, we develop a dry convective adjustment scheme for use in general circulation models (GCMs). This scheme relies on an energy analysis to determine the final adjusted atmospheric state. Our convection scheme produces results that agree with our CM1 simulations and can easily be implemented in GCMs to improve modeling of compositional convection in exoplanet atmospheres.
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Seager, Sara. "Exoplanet atmospheres: A theoretical outlook." Proceedings of the International Astronomical Union 6, S276 (October 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 hopes pinned on the James Webb Space Telescope, scheduled for launch in 2014. Further in the future lies direct imaging attempts to answer the enigmatic and ancient question, “Are we alone?” via atmospheric biosignatures.
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Krissansen-Totton, Joshua. "Implications of Atmospheric Nondetections for Trappist-1 Inner Planets on Atmospheric Retention Prospects for Outer Planets." Astrophysical Journal Letters 951, no. 2 (July 1, 2023): L39. http://dx.doi.org/10.3847/2041-8213/acdc26.

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Abstract JWST secondary eclipse observations of Trappist-1b seemingly disfavor atmospheres >∼1 bar since heat redistribution is expected to yield dayside emission temperature below the ∼500 K observed. Given the similar densities of Trappist-1 planets, and the theoretical potential for atmospheric erosion around late M dwarfs, this observation might be assumed to imply substantial atmospheres are also unlikely for the outer planets. However, the processes governing atmosphere erosion and replenishment are fundamentally different for inner and outer planets. Here, an atmosphere–interior evolution model is used to show that an airless Trappist-1b (and c) only weakly constrains stellar evolution, and that the odds of outer planets e and f retaining substantial atmospheres remain largely unchanged. This is true even if the initial volatile inventories of planets in the Trappist-1 system are highly correlated. The reason for this result is that b and c sit unambiguously interior to the runaway greenhouse limit, and so have potentially experienced ∼8 Gyr of X-ray and extreme ultraviolet–driven hydrodynamic escape; complete atmospheric erosion in this environment only weakly constrains stellar evolution and escape parameterizations. In contrast, e and f reside within the habitable zone, and likely experienced a comparatively short steam atmosphere during Trappist-1's pre-main sequence, and consequently complete atmospheric erosion remains unlikely across a broad swath of parameter space (e and f retain atmospheres in ∼98% of model runs). Naturally, it is still possible that all Trappist-1 planets formed volatile-poor and are all airless today. But the airlessness of b (and c) does not require this, and as such, JWST transit spectroscopy of e and f remains the best near-term opportunity to characterize the atmospheres of habitable zone terrestrial planets.
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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 primordial atmospheres at an embedded phase of evolution. We investigate effects of atmospheric interaction on the planetesimals (mass loss) and the atmosphere (heating/cooling). Methods. We used atmospheric parameters from a snapshot of time-dependent evolution simulations for embedded atmospheres and simulated purely radial, infall events of siliceous planetesimals in a 1D, explicit code. We implemented energy transfer between friction, radiation transfer by the atmosphere and the body, and thermal ablation; this gives us the possibility to examine the effects on the planetesimals and the atmosphere. Results. We find that a significant amount of gravitational energy is indeed dissipated into the atmosphere, especially for larger planetary cores, which consequently cannot contribute to the atmospheric planetary luminosity. Furthermore, we examine that planetesimal infall events for cores, MC > 2M⊕, which actually result in a local cooling of the atmosphere; this is totally in contradiction with the classical model.
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Ridden-Harper, Andrew, Stevanus K. Nugroho, Laura Flagg, Ray Jayawardhana, Jake D. Turner, Ernst de Mooij, Ryan MacDonald, et al. "High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b." Astronomical Journal 165, no. 4 (March 21, 2023): 170. http://dx.doi.org/10.3847/1538-3881/acbd39.

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Abstract Terrestrial exoplanets orbiting M-dwarf stars are promising targets for transmission spectroscopy with existing or near-future instrumentation. The atmospheric composition of such rocky planets remains an open question, especially given the high X-ray and ultraviolet flux from their host M dwarfs that can drive atmospheric escape. The 1.3 R ⊕ exoplanet GJ 486b (T eq ∼ 700 K), orbiting an M3.5 star, is expected to have one of the strongest transmission spectroscopy signals among known terrestrial exoplanets. We observed three transits of GJ 486b using three different high-resolution spectrographs: IRD on Subaru, IGRINS on Gemini-South, and SPIRou on the Canada–France–Hawai’i Telescope. We searched for atmospheric absorption from a wide variety of molecular species via the cross-correlation method, but did not detect any robust atmospheric signals. Nevertheless, our observations are sufficiently sensitive to rule out several clear atmospheric scenarios via injection and recovery tests, and extend comparative exoplanetology into the terrestrial regime. Our results suggest that GJ 486b does not possess a clear H2/He-dominated atmosphere, nor a clear 100% water-vapor atmosphere. Other secondary atmospheres with high mean molecular weights or H2/He-dominated atmospheres with clouds remain possible. Our findings provide further evidence suggesting that terrestrial planets orbiting M-dwarf stars may experience significant atmospheric loss.
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Chance, Quadry, Sarah Ballard, and Keivan Stassun. "Signatures of Impact-driven Atmospheric Loss in Large Ensembles of Exoplanets." Astrophysical Journal 937, no. 1 (September 1, 2022): 39. http://dx.doi.org/10.3847/1538-4357/ac8a97.

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Abstract The results of large-scale exoplanet transit surveys indicate that the distribution of small planet radii is likely sculpted by atmospheric loss. Several possible physical mechanisms exist for this loss of primordial atmospheres, each of which produces a different set of observational signatures. In this study, we investigate the impact-driven mode of atmosphere loss via N-body simulations. We compare the results from giant impacts, at a demographic level, to results from another commonly invoked method of atmosphere loss, photoevaporation. Applying two different loss prescriptions to the same sets of planets, we then examine the resulting distributions of planets with retained primordial atmospheres. As a result of this comparison, we identify two new pathways toward discerning the dominant atmospheric-loss mechanism at work. Both of these pathways involve using transit multiplicity as a diagnostic, in examining the results of follow-up atmospheric and radial velocity surveys.
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Watanabe, Yasuto, and Kazumi Ozaki. "Relative Abundances of CO2, CO, and CH4 in Atmospheres of Earth-like Lifeless Planets." Astrophysical Journal 961, no. 1 (January 1, 2024): 1. http://dx.doi.org/10.3847/1538-4357/ad10a2.

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Abstract Carbon is an essential element for life on Earth, and the relative abundances of major carbon species (CO2, CO, and CH4) in the atmosphere exert fundamental controls on planetary climate and biogeochemistry. Here we employed a theoretical model of atmospheric chemistry to investigate diversity in the atmospheric abundances of CO2, CO, and CH4 on Earth-like lifeless planets orbiting Sun-like (F-, G-, and K-type) stars. We focused on the conditions for the formation of a CO-rich atmosphere, which would be favorable for the origin of life. Results demonstrated that elevated atmospheric CO2 levels trigger photochemical instability of the CO budget in the atmosphere (i.e., CO runaway) owing to enhanced CO2 photolysis relative to H2O photolysis. Higher volcanic outgassing fluxes of reduced C (CO and CH4) also tend to initiate CO runaway. Our systematic examinations revealed that anoxic atmospheres of Earth-like lifeless planets could be classified in the phase space of CH4/CO2 versus CO/CO2, where a distinct gap in atmospheric carbon chemistry is expected to be observed. Our findings indicate that the gap structure is a general feature of Earth-like lifeless planets with reducing atmospheres orbiting Sun-like (F-, G-, and K-type) stars.
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Faxon, C. B., and D. T. Allen. "Chlorine chemistry in urban atmospheres: a review." Environmental Chemistry 10, no. 3 (2013): 221. http://dx.doi.org/10.1071/en13026.

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Environmental context Atmospheric chlorine radicals can affect the chemical composition of the atmosphere through numerous reactions with trace species. In urban atmospheres, the reactions of chlorine radicals can lead to effects such as increases in ozone production, thus degrading local and regional air quality. This review summarises the current understanding of atmospheric chlorine chemistry in urban environments and identifies key unresolved issues. Abstract Gas phase chlorine radicals (Cl•), when present in the atmosphere, react by mechanisms analogous to those of the hydroxyl radical (OH•). However, the rates of the Cl•-initiated reactions are often much faster than the corresponding OH• reactions. The effects of the atmospheric reactions of Cl• within urban environments include the oxidation of volatile organic compounds and increases in ozone production rates. Although concentrations of chlorine radicals are typically low compared to other atmospheric radicals, the relatively rapid rates of the reactions associated with this species lead to observable changes in air quality. This is particularly evident in the case of chlorine radical-induced localised increases in ozone concentrations. This review covers five aspects of atmospheric chlorine chemistry: (1) gas phase reactions; (2) heterogeneous and multi-phase reactions; (3) observational evidence of chlorine species in urban atmospheres; (4) regional modelling studies and (5) areas of uncertainty in the current state of knowledge.
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Radmilović-Radjenović, Marija, Martin Sabo, and Branislav Radjenović. "Transport Characteristics of the Electrification and Lightning of the Gas Mixture Representing the Atmospheres of the Solar System Planets." Atmosphere 12, no. 4 (March 29, 2021): 438. http://dx.doi.org/10.3390/atmos12040438.

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Electrification represents a fundamental process in planetary atmospheres, widespread in the Solar System. The atmospheres of the terrestrial planets (Venus, Earth, and Mars) range from thin to thick are rich in heavier gases and gaseous compounds, such as carbon dioxide, nitrogen, oxygen, argon, sodium, sulfur dioxide, and carbon monoxide. The Jovian planets (Jupiter, Saturn, Uranus, and Neptune) have thick atmospheres mainly composed of hydrogen and helium involving. The electrical discharge processes occur in the planetary atmospheres leading to potential hazards due to arcing on landers and rovers. Lightning does not only affect the atmospheric chemical composition but also has been involved in the origin of life in the terrestrial atmosphere. This paper is dealing with the transport parameters and the breakdown voltage curves of the gas compositions representing atmospheres of the planets of the Solar System. Ionization coefficients, electron energy distribution functions, and the mean energy of the atmospheric gas mixtures have been calculated by BOLSIG+. Transport parameters of the carbon dioxide rich atmospheric compositions are similar but differ from those of the Earth’s atmosphere. Small differences between parameters of the Solar System’s outer planets can be explained by a small abundance of their constituent gases as compared to the abundance of hydrogen. Based on the fit of the reduced effective ionization coefficient, the breakdown voltage curves for atmospheric mixtures have been plotted. It was found that the breakdown voltage curves corresponding to the atmospheres of Solar System planets follow the standard scaling law. Results of calculations satisfactorily agree with the available data from the literature. The minimal and the maximal value of the voltage required to trigger electric breakdown is obtained for the Martian and Jupiter atmospheres, respectively.
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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 (May 2, 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 predict the observability of each exoplanet’s atmosphere. TOI-270c and d are excellent targets for detecting atmospheres with JWST transmission spectroscopy, requiring only 1 transit observation with NIRISS, NIRSpec, and MIRI; higher signal-to-noise ratio can be obtained for a clear H-rich atmosphere. Fewer than three transits with NIRISS and NIRSpec may be enough to reveal molecular features. Water-dominated atmospheres require more transits. Water spectral features in water-dominated atmospheres may be detectable with NIRISS in two or three transits. We find that the detection of spectral features in a cloudy, H-rich atmosphere does not require integrations as long as those required for the water-dominated atmosphere, which is consistent with the differences in atmospheric mean molecular weight. TOI-270c and d could be prime targets for JWST transit observations of sub-Neptune atmospheres. These results provide useful predictions for observers who may propose to use JWST to detect and characterize the TOI-270 planet atmospheres.
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Dissertations / Theses on the topic "Atmospheric"

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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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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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Yang, Rena M. Arch Massachusetts Institute of Technology. "Atmospheric interventions." Thesis, Massachusetts Institute of Technology, 2015. http://hdl.handle.net/1721.1/97278.

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Thesis: M. Arch., Massachusetts Institute of Technology, Department of Architecture, 2015.
This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references (page 135).
Humans have been sheltering themselves from the harsh elements of their surroundings to maintain comfort since the discovery of the hearth. With the rise of the Industrial Revolution came innovations that made mitigating external conditions convenient and easy. The standard 70 degree Fahrenheit, with 30-candle-feet of illumination, 30-50% humidity, and ventilation became the norm and is replicated and placed regardless of existing conditions, creating homogeneous environments. Our conventional conception of the relationship between architecture and the environment is based on false assumptions that we reside comfortably in the standard air-conditioned 70 degrees, effectively producing desensitizing spaces. For a body to understand and experience space, it is important for these environments to have an atmospheric affect that is absorbed through the senses. Architecture is then seen as a stimulus by provoking and challenging the body and creating a consciousness of body and environment. This thesis states that the sensorial appreciation in architecture can be explored through sequenced and curated experiences of architecture to use, amplify and appease the senses. This creates new atmospheric conditions conceived of relative sequencing and juxtapositions, rather than appeasing and mediating the existing environment. This idea is explored through three interventions on the Harvard Bridge in Boston, Massachusetts that seeks to engage the hostile environmental conditions.
by Rena Yang.
M. Arch.
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Lehtola, Amanda M. "Atmospheric Biomorphism." Kent State University / OhioLINK, 2008. http://rave.ohiolink.edu/etdc/view?acc_num=kent1208803878.

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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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Dionne, Pierre 1962. "Numerical simulation of blocking by the resonance of topographically forced waves." Thesis, McGill University, 1986. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=65542.

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Holley, Rachel. "Mitigating Atmospherics Path Delays in Radar Interferometry Over Volcanoes - Atmospheric Modelling and Persistent." Thesis, University of Reading, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.519864.

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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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Sefcik, Lesley T. "Biophere-atmosphere interactions : Northern hardwood seedling responses to anthropogenic atmospheric resource alteration /." Saarbrücken : VDM Verlag Dr. Müller, 2008. http://d-nb.info/988972131/04.

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Robertson, Lynette B. "Radon emissions to the atmosphere and their use as an atmospheric tracer." Thesis, University of Edinburgh, 2004. http://hdl.handle.net/1842/14311.

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The naturally-occurring radioactive gases 222Rn and 220Rn are widely used as atmospheric tracers in a variety of applications pertinent to climate and air quality studies, but their use in this context is currently limited by poor knowledge of the spatial and temporal pattern in emissions. The aim of this research was to improve knowledge of 222Rn and 220Rn emissions by investigating their spatial and temporal variation in emissions on various scales. Novel approaches to measuring 222Rn and 220Rn fluxes by the closed chamber method have been developed and compared with some existing methods, and studies of some controlling variables for which there is limited and conflicting information (water table depth, freezing of the soil and snow cover) have been carried out. Studies of the short-term variability in 222Rn emissions made with an automatic chamber showed that outside periods of rain the 222Rn flux was relatively constant (CV = ~ 25 %), but heavy rainfall may temporarily completely suppress the radon flux if the soil surface becomes saturated. On the seasonal time-scale, flux measurements made on a medium- moisture was found to be the most important factor controlling the variations in radon flux; air pressure and temperature were not important. Field measurements and a laboratory study using a soil monolith showed that water table depth was also an important factor for 222Rn flux, but not for 220Rn, due to its much shorter diffusion length. Freezing of the soil surface layer (~ 5cm depth) did not cause a significant reduction in 222Rn or 220Rn flux. Studies of the spatial variability of 222Rn emissions at the local scale showed that 222Rn flux is approximately normally distributed (CV = 55 %), and that soil moisture is an important factor. However, measurements made at 15 sites of different soil type and geology across North Britain showed 222Rn emissions to be log-normally distributed at this larger scale and highly variable (CV = ~ 200%). The 226Ra content of the soil, which ranged from <3 Bq kg-1 to 55 Bq kg-1 was found to account for a large proportion of the observed variability (~ 80 %). The median 222Rn flux was 9.7 Bq m-2 h-1, indicating that the average flux from this region is considerably lower than the global average, as would be expected given the large proportion of peat soils and generally high soil water content and shallow water tables. A 222Rn flux map produced for North Britain using a GIS and empirical model based on soil and geology classifications was able to reproduce the main spatial pattern in emissions, but on the whole, significantly under- predicted the magnitude of fluxes.
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Books on the topic "Atmospheric"

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Justus, C. G. The NASA/MSFC Global Reference Atmospheric Model--1999 version (GRAM-99). [Marshall Space Flight Center], Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 1999.

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Justus, C. G. The NASA/MSFC Global Reference Atmospheric Model--1999 version (GRAM-99). [Marshall Space Flight Center], Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 1999.

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Justus, C. G. The NASA/MSFC Global Reference Atmospheric Model--1999 version (GRAM-99). [Marshall Space Flight Center], Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 1999.

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Yiğit, Erdal. Atmospheric and Space Sciences: Neutral Atmospheres. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-21581-5.

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Daley, Roger. Atmospheric data analysis. Cambridge: Cambridge University Press, 1991.

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Center, Goddard Space Flight, ed. Mesoscale Atmospheric Processes Branch: Laboratory for Atmospheres. Greenbelt, Md: Goddard Space Flight Center, 1996.

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Center, Goddard Space Flight, ed. Mesoscale Atmospheric Processes Branch: Laboratory for Atmospheres. Greenbelt, Md: Goddard Space Flight Center, 1996.

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Center, Goddard Space Flight, ed. Mesoscale Atmospheric Processes Branch: Laboratory for Atmospheres. Greenbelt, Md: Goddard Space Flight Center, 1996.

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Center, Goddard Space Flight, ed. Mesoscale Atmospheric Processes Branch: Laboratory for Atmospheres. Greenbelt, Md: Goddard Space Flight Center, 1996.

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F, Leblanc, ed. Planetary atmospheric electricity. [New York?]: Springer, 2008.

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Book chapters on the topic "Atmospheric"

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Wolf, Barbara. "Atmospheres of Learning, Atmospheric Competence." In Atmosphere and Aesthetics, 209–21. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-24942-7_12.

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Manahan, Stanley E. "The Atmosphere and Atmospheric Chemistry." In Environmental Chemistry, 205–36. 11th ed. Boca Raton: CRC Press, 2022. http://dx.doi.org/10.1201/9781003096238-8.

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Rasch, Philip J. "Atmospheric General Circulation Modeling atmosphere/atmospheric general circulation modeling (AGCM)." In Encyclopedia of Sustainability Science and Technology, 622–38. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4419-0851-3_354.

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Yiğit, Erdal. "Introduction to Atmospheric Physics." In Atmospheric and Space Sciences: Neutral Atmospheres, 9–28. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-21581-5_2.

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Yiğit, Erdal. "Atmospheric Circulation and Dynamical Processes." In Atmospheric and Space Sciences: Neutral Atmospheres, 81–99. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-21581-5_6.

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Zimmermann, Felix. "Conclusion: Toward an Atmospherology of Digital Games." In Mental Health | Atmospheres | Video Games, 243–54. Bielefeld, Germany: transcript Verlag, 2022. http://dx.doi.org/10.14361/9783839462645-018.

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This concluding chapter outlines an atmospherology of digital games. It is argued that atmospheres bring with them distinct terminological challenges which a game atmospherology would have to tackle. Summarizing core arguments brought forth by the authors in this book, this chapter concludes that researchers should come to terms with the inescapable vagueness of the common discourse surrounding atmospheres. It is suggested that atmosphere could constitute an umbrella term under which other terms like ambience, mood, or tone can be subsumed, with each term providing a specific focus and nuanced view of atmospheric experience.
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Zhang, Xiaoge Gregory. "Atmospheric Corrosion." In Corrosion and Electrochemistry of Zinc, 241–81. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4757-9877-7_8.

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Surkov, Vadim, and Masashi Hayakawa. "Atmospheric Electricity." In Ultra and Extremely Low Frequency Electromagnetic Fields, 57–106. Tokyo: Springer Japan, 2014. http://dx.doi.org/10.1007/978-4-431-54367-1_3.

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Spiridonov, Vlado, and Mladjen Curic. "Atmospheric Moisture." In Fundamentals of Meteorology, 123–33. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-52655-9_10.

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Spiridonov, Vlado, and Mladjen Ćurić. "Atmospheric Motion." In Fundamentals of Meteorology, 159–95. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-52655-9_12.

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Conference papers on the topic "Atmospheric"

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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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Longo, Francesco, and Giovanni Laneve. "Iterative atmospheric parameters estimation of the tropical atmosphere." In Remote Sensing, edited by Klaus Schaefer, Adolfo Comeron, Michel R. Carleer, and Richard H. Picard. SPIE, 2004. http://dx.doi.org/10.1117/12.511007.

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Chadwick, P. M. "Atmospheric sensing for atmospheric Cherenkov telescopes." In The international symposium on high energy gamma-ray astronomy. AIP, 2001. http://dx.doi.org/10.1063/1.1370832.

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Vermote, E., G. Doxani, F. Gascon, and J. C. Roger. "ACIX – Atmospheric Atmospheric Correction Inter-comparison eXercise." In IGARSS 2019 - 2019 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2019. http://dx.doi.org/10.1109/igarss.2019.8900457.

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Goldsmith, J. E. M., and Scott E. Bisson. "Raman Lidar Profiling of Atmospheric Water Vapor." In Laser Applications to Chemical Analysis. Washington, D.C.: Optica Publishing Group, 1994. http://dx.doi.org/10.1364/laca.1994.wc.2.

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Detailed measurements of the distribution of water vapor in the atmosphere are needed for a variety of scientific inquiries, including global climate change and related issues in radiative processes (water vapor is the major greenhouse gas in the atmosphere), and studies of a variety of atmospheric processes such as cloud formation and atmospheric circulation. The Raman lidar is a leading candidate for an instrument capable of the detailed, time- and space-resolved measurements required by these and other studies.
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Borsilov, Alexander, Denis V. Kazakov, Petr A. Konyaev, Vladimir P. Lukin, Egor L. Soin, and Andrey V. Torgaev. "Optical and acoustic measurements of atmospheric turbulence on horizontal paths in the atmosphere." In XXIX International Symposium "Atmospheric and Ocean Optics, Atmospheric Physics", edited by Oleg A. Romanovskii. SPIE, 2023. http://dx.doi.org/10.1117/12.2688114.

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Manninen, Hanna E., Hannes Tammet, Antti Mäkelä, Jussi Haapalainen, Sander Mirme, Tuomo Nieminen, Alessandro Franchin, Tuukka Petäjä, Markku Kulmala, and Urmas Hõrrak. "Atmospheric electricity and aerosol-cloud interactions in earth’s atmosphere." In NUCLEATION AND ATMOSPHERIC AEROSOLS: 19th International Conference. AIP, 2013. http://dx.doi.org/10.1063/1.4803390.

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Yadav, Atul, and R. K. Giri. "Atmospheric physics advancements: Modelling the aerosols in the atmosphere." In NATIONAL CONFERENCE ON RECENT ADVANCES IN EXPERIMENTAL AND THEORETICAL PHYSICS (RAETP-2018). Author(s), 2018. http://dx.doi.org/10.1063/1.5051305.

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Hays, Paul B. "Remote Sensing of Atmospheric Winds." In Optical Remote Sensing. Washington, D.C.: Optica Publishing Group, 1985. http://dx.doi.org/10.1364/ors.1985.wa3.

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The technique for measuring atmospheric winds from the Upper Atmosphere Research Satellite (UARS) is discussed. Stress is placed on the use of absorption features in the spectrum of scattered sunlight to measure the motion of the atmosphere by doppler techniques. Instrumental detail will be presented for the High Resolution Doppler Imager (HRDI) which will be used to make the observations of winds from the UARS.
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KANEYUKI, K. "ATMOSPHERIC NEUTRINOS." In Physics in Collision 19. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792648_0015.

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Reports on the topic "Atmospheric"

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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), March 2007. http://dx.doi.org/10.2172/900475.

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Yoo, J., and G. Kim. Atmospheric observations. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2015. http://dx.doi.org/10.4095/295973.

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Jin, K. H. Atmospheric observations. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2016. http://dx.doi.org/10.4095/297877.

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Hodur, Richard M. Atmospheric Models. Fort Belvoir, VA: Defense Technical Information Center, September 1997. http://dx.doi.org/10.21236/ada629034.

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Hyman, Ellis, Roger Shi, Mark Czarnaski, and Sethu Raman. Atmospheric Forecasting. Fort Belvoir, VA: Defense Technical Information Center, October 2000. http://dx.doi.org/10.21236/ada384012.

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Park, J., Y. Kim, C. K. Lim, L. Peng, and Y. Li. Atmospheric observations. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2018. http://dx.doi.org/10.4095/308408.

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Hammel, Stephen, Dimitri Tsintikidis, and Alexander M. van Eijk. Atmospheric Optical Propagation. Fort Belvoir, VA: Defense Technical Information Center, September 2008. http://dx.doi.org/10.21236/ada532877.

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Sprangle, Phillip, Joseph Penano, Bahman Hafizi, Daniel Gordon, and Marlan Scully. Remote Atmospheric Lasing. Fort Belvoir, VA: Defense Technical Information Center, September 2010. http://dx.doi.org/10.21236/ada536426.

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Laroussi, Mounir. Atmospheric Plasma Research. Fort Belvoir, VA: Defense Technical Information Center, July 2001. http://dx.doi.org/10.21236/ada388908.

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Hammel, Stephen, Dimitri Tsintikidis, and Alexander M. Van Eijk. Atmospheric Optical Propagation. Fort Belvoir, VA: Defense Technical Information Center, September 2007. http://dx.doi.org/10.21236/ada548345.

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