Relevant bibliographies by topics / Atmosphere interactions

Academic literature on the topic 'Atmosphere interactions'

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Published: 4 June 2021
Last updated: 29 January 2023

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Journal articles on the topic "Atmosphere interactions"

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Fowler, D., K. Pilegaard, M. A. Sutton, P. Ambus, M. Raivonen, J. Duyzer, D. Simpson, et al. "Atmospheric composition change: Ecosystems–Atmosphere interactions." Atmospheric Environment 43, no. 33 (October 2009): 5193–267. http://dx.doi.org/10.1016/j.atmosenv.2009.07.068.

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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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Lellouch, Emmanuel. "Io’s Atmosphere and Surface-Atmosphere Interactions." Space Science Reviews 116, no. 1-2 (January 2005): 211–24. http://dx.doi.org/10.1007/s11214-005-1957-z.

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Costa, Marcos Heil, Michael T. Coe, and David R. Galbraith. "Land-Atmosphere Interactions." Advances in Meteorology 2016 (2016): 1. http://dx.doi.org/10.1155/2016/2362398.

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Curtis, Peter S. "Biosphere-atmosphere interactions." New Phytologist 162, no. 1 (April 2004): 4–6. http://dx.doi.org/10.1111/j.1469-8137.2004.01044.x.

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Potter, Brian E. "Atmospheric interactions with wildland fire behaviour - I. Basic surface interactions, vertical profiles and synoptic structures." International Journal of Wildland Fire 21, no. 7 (2012): 779. http://dx.doi.org/10.1071/wf11128.

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This paper is the first of two reviewing scientific literature from 100 years of research addressing interactions between the atmosphere and fire behaviour. These papers consider research on the interactions between the fuels burning at any instant and the atmosphere, and the interactions between the atmosphere and those fuels that will eventually burn in a given fire. This first paper reviews the progression from the surface atmospheric properties of temperature, humidity and wind to horizontal and vertical synoptic structures and ends with vertical atmospheric profiles. (The companion paper addresses plume dynamics and vortices.) The review reveals several unanswered questions, as well as findings from previous studies that appear forgotten in current research and concludes with suggestions for areas of future research.
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Potter, Brian E. "A dynamics based view of atmosphere - fire interactions." International Journal of Wildland Fire 11, no. 4 (2002): 247. http://dx.doi.org/10.1071/wf02008.

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Current research on severe fire interactions with the atmosphere focuses largely on examination of correlations between fire growth and various atmospheric properties, and on the development of indices based on these correlations. The author proposes that progress requires understanding the physics and atmospheric dynamics behind the correlations. A conceptual 3-stage model of fire development, based on atmospheric structure, is presented. Using parcel theory and basic atmospheric dynamics equations, the author proposes possible causal explanations for some of the known correlations. The atmospheric dynamics are discussed in terms of the 3-stage model, but can also be viewed more generally. The overall goal is to reframe fire–atmosphere interactions in a way that will allow better understanding and progress in fire science, prediction, and safety.
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Johnstone, Colin P. "The Influences of Stellar Activity on Planetary Atmospheres." Proceedings of the International Astronomical Union 12, S328 (October 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 star's output and the time dependent properties of the planet's atmosphere.
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Waite, J. H., R. S. Perryman, M. E. Perry, K. E. Miller, J. Bell, T. E. Cravens, C. R. Glein, et al. "Chemical interactions between Saturn’s atmosphere and its rings." Science 362, no. 6410 (October 4, 2018): eaat2382. http://dx.doi.org/10.1126/science.aat2382.

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The Pioneer and Voyager spacecraft made close-up measurements of Saturn’s ionosphere and upper atmosphere in the 1970s and 1980s that suggested a chemical interaction between the rings and atmosphere. Exploring this interaction provides information on ring composition and the influence on Saturn’s atmosphere from infalling material. The Cassini Ion Neutral Mass Spectrometer sampled in situ the region between the D ring and Saturn during the spacecraft’s Grand Finale phase. We used these measurements to characterize the atmospheric structure and material influx from the rings. The atmospheric He/H2 ratio is 10 to 16%. Volatile compounds from the rings (methane; carbon monoxide and/or molecular nitrogen), as well as larger organic-bearing grains, are flowing inward at a rate of 4800 to 45,000 kilograms per second.
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Itcovitz, Jonathan P., Auriol S. P. Rae, Robert I. Citron, Sarah T. Stewart, Catriona A. Sinclair, Paul B. Rimmer, and Oliver Shorttle. "Reduced Atmospheres of Post-impact Worlds: The Early Earth." Planetary Science Journal 3, no. 5 (May 1, 2022): 115. http://dx.doi.org/10.3847/psj/ac67a9.

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Abstract Impacts may have had a significant effect on the atmospheric chemistry of the early Earth. Reduced phases in the impactor (e.g., metallic iron) can reduce the planet’s H2O inventory to produce massive atmospheres rich in H2. While previous studies have focused on the interactions between the impactor and atmosphere in such scenarios, we investigate two further effects: (1) the distribution of the impactor’s iron inventory during impact between the target interior, target atmosphere, and escaping the target; and (2) interactions between the post-impact atmosphere and the impact-generated melt phase. We find that these two effects can potentially counterbalance each other, with the melt–atmosphere interactions acting to restore reducing power to the atmosphere that was initially accreted by the melt phase. For a ∼1022 kg impactor, when the iron accreted by the melt phase is fully available to reduce this melt, we find an equilibrium atmosphere with H2 column density ∼104 moles cm−2 (pH2 ∼ 120 bars, X H2 ∼ 0.77), consistent with previous estimates. However, when the iron is not available to reduce the melt (e.g., sinking out in large diameter blobs), we find significantly less H2 (7 × 102 − 5 × 103 moles cm−2, pH2 ≲ 60 bars, X H2 ≲ 0.41). These lower H2 abundances are sufficiently high that species important to prebiotic chemistry can form (e.g., NH3, HCN), but sufficiently low that the greenhouse heating effects associated with highly reducing atmospheres, which are problematic to such chemistry, are suppressed. The manner in which iron is accreted by the impact-generated melt phase is critical in determining the reducing power of the atmosphere and resolidified melt pool in the aftermath of impact.
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Dissertations / Theses on the topic "Atmosphere interactions"

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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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Grant, Eleanor Rose. "Canopy-atmosphere interactions over complex terrain." Thesis, University of Leeds, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.550799.

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The study of boundary layer flow through a forest canopy on complex terrain has, until recently, been limited to modelling and laboratory studies. This thesis presents a unique set of field measurements from within and above a canopy situated on a ridge. A climatological study of the observed dataset is presented to identify the significant fea- tures of these flows that differentiate them from air flows above and within a homogeneous canopy on flat terrain. The ridge is found to impact on the flows in the following ways. On the summit the velocity profile resembles that of a canopy profile on flat terrain with little variation in wind.speed below the canopy and an obvious inflection point at the canopy top. On the windward slope, the inflection point disappears. Significant amounts of -u'w' at the canopy top indicates that turbulent mixing acts strongly to transport higher mo- mentum air down into the canopy, which smooths the layer of shear. The profile on the lee slope is dependent on the size of a separation region that can develop on the lee slope of the forested ridge. The direction of the mean wind within the canopy on the lee slope is dependent on the hill-induced pressure gradient, which tends to drive a reversed flow up the lee slope, and on the turbulent mixing which tends to drive the flow down-slope through the mixing of higher momentum air from above the canopy. If the hill slope is sufficiently large (so the pressure gradient is large), or the canopy is sufficiently deep (so that turbulence is unable to mix the higher momentum air all the way to the bottom), then flow separation can occur. Case studies are presented to investigate the formation and development of the separation region on the lee slope of the forested ridge. The presence of a flow separation region is observed to extend the width of the dynamic pressure profile such that, as the separation region expands up the lee slope towards the summit, the minimum is forced back to the upwind edge of the separation region. Large scale separation is observed on the ridge, whereby the separation region extends beyond the top of the canopy. Within the separation region, there is little variation in wind speed or vertical momentum flux with height as the inflection point is elevated to the top of the separation region. Comparisons between the observed case studies and model simulations are made to quan- tify the success of the model at simulating canopy air flows over complex terrain. The model is found to successfully capture the main features the these flows. Areas where the model was less successful are attributed to the inhomogeneous nature of the canopy and the terrain at the field site, and to the low resolution of the model.
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Goodman, Jason (Jason Curtis) 1973. "Interannual middle-latitude atmosphere-ocean interactions." Thesis, Massachusetts Institute of Technology, 2001. http://hdl.handle.net/1721.1/16779.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2001.
Includes bibliographical references (p. 144-151).
This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
This thesis discusses the interaction of atmosphere and ocean in midlatitudes on interannual and decadal timescales. We investigate the extent to which mutuallycoupled atmosphere-ocean feedback can explain the observed coupled variability on these timescales, and look for preferred modes of atmospheric response to forcing by sea-surface temperature anomalies. First, we formulate and study a very simple analytical model of the mutual interaction of the middle-latitude atmosphere and ocean. The model is found to support coupled modes in which oceanic baroclinic Rossby waves of decadal period grow through positive coupled feedback between the thermal forcing of the atmosphere induced by associated SST anomalies and the resulting windstress forcing of the ocean. Growth only occurs if the atmospheric response to thermal forcing is equivalent barotropic, with a particular phase relationship with the underlying SST anomalies. The dependence of the growth rate and structure of the modes on the nature of the assumed physics of air-sea interaction is explored, and their possible relation to observed phenomena discussed. We then construct a numerical model with the same physics; this enables us to consider the effects of nontrivial boundary conditions and background flows within the model. We find that the finite fetch of a closed ocean basin reduces growth rate and can lead to decay. However, the coupled mode described above remains the least-damped, and is thus the pattern most easily energized by stochastic forcing. Using a non-uniform atmospheric background flow focuses perturbation energy into particular areas, so that the coupled mode's expression in the atmosphere becomes fixed in space, rather than propagating. This improves the mode's resemblance to observed patterns of variability, such as the North Atlantic Oscillation, which are generally stationary patterns which fluctuate in intensity. The atmospheric component of the coupled mode exists in a balance between Rossby-wave propagation and vorticity advection. This is the same balance as the "neutral vectors" described by Marshall and Molteni (1993). Neutral vectors are the right singular vectors of the linearized atmospheric model's tendency matrix that have the smallest eigenvalues; they are also the patterns that exhibit the largest response to forcing perturbations in the linear model. We explain how the coupled mode arises as the ocean excites atmospheric neutral vectors. Neutral vectors act as pattern-specific amplifiers of ocean SST anomalies. We then proceed to study the neutral vectors of a quasigeostrophic model with realistic mean flow. We find a striking similarity between these patterns and the dominant patterns of variability observed in both the full nonlinear model and in the real world. We provide a mathematical explanation for this connection. Investigation of the "optimal forcing patterns" - the left singular vectors - proves to be less fruitful. The neutral modes have equivalent barotropic vertical structure, but their optimal forcing patterns are baroclinic and seem to be associated with low level heating. But the horizontal patterns of the forcing patterns are not robust, and are sensitive to the form of the inner product used in the SVD analysis. Additionally, applying "optimal" forcing patterns as perturbations to the full nonlinear model does not generate the response suggested by the linear model.
by Jason Goodman.
Ph.D.
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Shannon, Debbie Anne. "Atmosphere-vegetation interactions over South Africa." Master's thesis, University of Cape Town, 1997. http://hdl.handle.net/11427/22109.

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Bibliography: pages 107-118.
This study examines the sensitivity of the atmospheric circulation to vegetation change over South Africa in the context of the portended global warming. This is achieved using a vegetation model driven by climate change information and subsequently incorporated within a general circulation model (GCM). The stand-alone vegetation model is driven using precipitation, temperature and relative humidity derived from downscaling using artificial neural networks. The vegetation model is then run with perturbed precipitation, temperature and relative humidity from downscaled model data from lxCO₂ and 2xCO₂ GCM simulations. The resultant vegetation perturbation response to climate change is then examined and incorporated into the GCM in order to ascertain the atmospheric sensitivity to vegetation changes. The off-line results of the vegetation model indicate a moderate degree of sensitivity of the vegetation to perturbations in precipitation, temperature and relative humidity. The general trend in response to the CO₂ climate is a westwards and altitudinal shift of lowland vegetation over the eastern part of the country, and a southwards and eastwards shift of the more dryland vegetation in the west. These shifts are in accordance with expected responses, since lowland vegetation responds more to temperature changes and the dryland vegetation to precipitation changes. Nonetheless, the use of the model provides a physically justifiable scenario on which to base the GCM studies, and at a finer resolution than otherwise available. A GCM simulation with the perturbed vegetation was then performed using sea surface temperature boundary conditions for 1980 and compared to an identical GCM run without the perturbation. 1980 was chosen since this year does not represent either a strong El Niño or La Niña year. The atmospheric sensitivity to the vegetation perturbation has been examined in terms of climatic variables such as temperature, precipitation, pressure, specific humidity, horizontal divergence, and sensible and latent heat fluxes. The results show that the atmosphere is quite sensitive to relatively small vegetation changes. Atmospheric response to vegetation perturbations indicates greater sensitivity over the NW and SE regions of southern Africa. The perturbation indicates a reduction in precipitation over the SE interior, related to less moisture feeding in over the interior from the SE Indian Ocean. Wind speed changes over the adjacent ocean were also evident, and are probably related to the changes in the South Atlantic and Indian high pressures. A southwards extension of the Hadley Cell was also suggested, as well as changes in sensible and latent heat fluxes, relating to precipitation and temperature changes. It is suggested that changes may be in response to the general drying out of the country and the associated increase in aridity. This research forms the preliminary investigation for further work incorporating the atmospheric perturbation response back into driving the vegetation model in order to examine the direction of the feedback -- whether this is positive or negative in the longer term. Thus, this study has demonstrated that the atmosphere is significantly sensitive to vegetation changes over South Africa and reinforces the need for improved land surface parameterization schemes and vegetation models in general circulation models.
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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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Simonot, Jean-Yves. "Contributions a l'etude des interactions ocean-atmosphere." Paris 6, 1988. http://www.theses.fr/1988PA066541.

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En vue du couplage avec un modele de la circulation generale atmospherique, pour realiser des experiences de simulation du climat et de ses changements, un modele de couche melangee oceanique global a ete developpe comprenant une modelisation de la turbulence integree sur les couches superficielles de l'ocean, un schema de transport horizontal du contenu thermique par des courants et une diffusion climatiques prescrits, une parametrisation du pompage d'ekman et de l'upwelling equatorial. En mode local, le modele est utilise pour simuler deux cycles saisonniers de temperature de surface au point meteorologique r, ainsi que pour evaluer l'impact de la retro-action thermique, via les proprietes optiques, due a une simulation du cycle saisonnier de phytoplancton. Des etudes de climatologie des flux de surface necessaires au forcage du modele ont ete realisees en analysant plusieurs annees de champs journaliers predits quotidiennement par un modele de prevision operationnelle du temps. Ces etudes ont permis de mettre en evidence des biais systematiques du modele, mais ont aussi montre que ces champs contiennent une information climatologique non negligeable. Enfin, des methodes satellitaires ont ete utilisees afin de produire des champs de flux de surface. Les resultats montrent une grande imprecision sur ces methodes avec les capteurs actuels, mais demontrent leur grande potentialite en ce qui concerne les capteurs en cours de developpement
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Kala, Jatin. "Land-atmosphere interactions in Southwest Western Australia." Thesis, Kala, Jatin ORCID: 0000-0001-9338-2965 (2011) Land-atmosphere interactions in Southwest Western Australia. PhD thesis, Murdoch University, 2011. https://researchrepository.murdoch.edu.au/id/eprint/10624/.

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The Southwest of Western Australia (SWWA) is a region of extensive land cover change with an estimated 13 million hectares of native vegetation cleared since European settlement. Whilst previous studies have suggested meteorological and climatological implications of this change in land use, no studies have explicitly focussed on the detailed mechanisms behind the impacts of land-cover change on individual meteorological phenomena. This thesis seeks to identify the physical mechanisms inducing changes within the atmosphere by using the Regional Atmospheric Modeling System (RAMS V6.0) to simulate the impact of land use change on meteorological phenomena at different scales and evaluate these model results against high resolution atmospheric soundings, station observations, and gridded rainfall analyses where appropriate. Sensitivity tests show that land-cover change results in an increase in low-level atmospheric moisture advection associated with the southern sea-breeze due to a reduction in surface roughness. It also results in a decrease in convective precipitation associated with cold-fronts and convective clouds associated with the surface heat trough, due to an increase in wind speed, and a decrease in turbulent kinetic energy and vertically integrated moisture convergence within the PBL. Large-eddy simulations further highlight the role of land-cover change and soil moisture, as well as the contributions of surface versus entrainment fluxes on the growth of the PBL and development of convective clouds. These results are discussed within the broader context of the meteorology of the region.
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Mohr, Karen Irene. "An investigation of land/atmosphere interactions : soil moisture, heat fluxes, and atmospheric convection /." Digital version:, 2000. http://wwwlib.umi.com/cr/utexas/fullcit?p9992875.

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Virmani, Jyotika I. "Ocean-atmosphere interactions on the West Florida shelf." [Tampa, Fla.] : University of South Florida, 2005. http://purl.fcla.edu/fcla/etd/SFE0001141.

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Books on the topic "Atmosphere interactions"

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1931-, Toba Y., ed. Ocean-atmosphere interactions. Tokyo: Terra Scientific Pub. Co., 2003.

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Shutter, Joshua, and Frank Keutsch. Biosphere-Atmosphere Interactions. Washington, DC, USA: American Chemical Society, 2021. http://dx.doi.org/10.1021/acsinfocus.7e5007.

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Liss, Peter S., and Martin T. Johnson, eds. Ocean-Atmosphere Interactions of Gases and Particles. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-25643-1.

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Wood, Eric F., ed. Land Surface — Atmosphere Interactions for Climate Modeling. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-009-2155-9.

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Liss, Peter S. Ocean-Atmosphere Interactions of Gases and Particles. Cham: Springer Nature, 2014.

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NATO Advanced Workshop on Regional and Global Ozone Interaction and its Environmental Consequences (1987 Lillehammer, Norway). Tropospheric ozone: Regional and global scale interactions. Dordrecht: D. Reidel Pub. Co., 1988.

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Lowry, William P. Fundamentals of biometeorology: Interactions of organisms and the atmosphere. St Louis, Miss: Peavine Publications, 2001.

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Lowry, William P. Fundamentals of biometeorology: Interactions of organisms and the atmosphere. Minnville, Oregon: Peavine, 1989.

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Garstang, Michael. Observations of surface to atmosphere interactions in the tropics. New York: Oxford University Press, 1999.

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S, Jacobs Stanley, and Weiss Ray F, eds. Ocean, ice, and atmosphere: Interactions at the Antarctic continental margin. Washington, D.C: American Geophysical Union, 1998.

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Book chapters on the topic "Atmosphere interactions"

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Pielke, R. A., T. N. Chase, J. Eastman, L. Lu, G. E. Liston, M. B. Coughenour, D. Ojima, W. J. Parton, and T. G. F. Kittel. "Land-Atmosphere Interactions." In Advances in Global Change Research, 119–26. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/0-306-48051-4_13.

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Eymard, Laurence, and Gilles Reverdin. "Ocean-Atmosphere Interactions." In Ocean in the Earth System, 105–44. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2014. http://dx.doi.org/10.1002/9781119007678.ch3.

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Stocker, Thomas. "Atmosphere–Ocean Interactions." In Introduction to Climate Modelling, 137–50. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-00773-6_8.

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Scholes, Mary C., Patricia A. Matrai, Meinrat O. Andreae, Keith A. Smith, Martin R. Manning, Paulo Artaxo, Leonard A. Barrie, et al. "Biosphere-Atmosphere Interactions." In Atmospheric Chemistry in a Changing World, 19–71. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/978-3-642-18984-5_2.

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Fisher, Joshua B. "Land-Atmosphere Interactions, Evapotranspiration." In Encyclopedia of Remote Sensing, 325–28. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-0-387-36699-9_82.

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Henderson-Sellers, A. "Archaean Atmosphere-Biosphere Interactions." In Climate and Geo-Sciences, 21–38. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2446-8_2.

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Vihma, Timo. "Atmosphere-Snow/Ice Interactions." In Encyclopedia of Earth Sciences Series, 66–75. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-90-481-2642-2_31.

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Jenkins, Mary Ann. "Coupled Fire-Atmosphere Interactions." In Encyclopedia of Wildfires and Wildland-Urban Interface (WUI) Fires, 1–15. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-319-51727-8_77-1.

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Jenkins, Mary Ann. "Coupled Fire-Atmosphere Interactions." In Encyclopedia of Wildfires and Wildland-Urban Interface (WUI) Fires, 165–80. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-319-52090-2_77.

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de Leeuw, Gerrit, Cécile Guieu, Almuth Arneth, Nicolas Bellouin, Laurent Bopp, Philip W. Boyd, Hugo A. C. Denier van der Gon, et al. "Ocean–Atmosphere Interactions of Particles." In Ocean-Atmosphere Interactions of Gases and Particles, 171–246. Berlin, Heidelberg: Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-25643-1_4.

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Conference papers on the topic "Atmosphere interactions"

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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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Sinha, Parikhit, William Hayes, and Lauren Ngan. "Regional atmosphere-solar PV interactions." In 2014 IEEE 40th Photovoltaic Specialists Conference (PVSC). IEEE, 2014. http://dx.doi.org/10.1109/pvsc.2014.6925197.

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da Silva, Jonatan J., Fábio J. S. Lopes, and Eduardo Landulfo. "Cloud-Aerosols interactions by multiple scenarios approach." In Remote Sensing of Clouds and the Atmosphere, edited by Adolfo Comerón, Evgueni I. Kassianov, and Klaus Schäfer. SPIE, 2017. http://dx.doi.org/10.1117/12.2278588.

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MacKenzie, Shannon, and Jason W. Barnes. "TITAN'S EVAPORITES: INVESTIGATING SURFACE-ATMOSPHERE INTERACTIONS IN TIME." In 68th Annual Rocky Mountain GSA Section Meeting. Geological Society of America, 2016. http://dx.doi.org/10.1130/abs/2016rm-276171.

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Kristensen, Steen Savstrup, Irfan Kuvvetli, Torsten Neubert, Carol Anne Oxborrow, Soren Moller Pedersen, Josef Polny, Ib Lundgaard Rasmussen, et al. "Atmosphere-Space Interactions Monitor, Instrument and First Results." In IGARSS 2019 - 2019 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2019. http://dx.doi.org/10.1109/igarss.2019.8900301.

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BATTISTONI, G., A. FERRARI, and P. R. SALA. "CALCULATION OF SECONDARY PARTICLES IN ATMOSPHERE AND HADRONIC INTERACTIONS." In Proceedings of the Second International Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776808_0016.

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Greenwood, Jhamieka, Bryan Quaife, and Kevin Speer. "A GPU-Accelerated Hydrodynamics Solver For Atmosphere-Fire Interactions." In SIGGRAPH '22: Special Interest Group on Computer Graphics and Interactive Techniques Conference. New York, NY, USA: ACM, 2022. http://dx.doi.org/10.1145/3532719.3543263.

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Cronin, Meghan F., Meghan F. Cronin, Meghan F. Cronin, Meghan F. Cronin, Meghan F. Cronin, Meghan F. Cronin, Meghan F. Cronin, et al. "Monitoring Ocean - Atmosphere Interactions in Western Boundary Current Extensions." In OceanObs'09: Sustained Ocean Observations and Information for Society. European Space Agency, 2010. http://dx.doi.org/10.5270/oceanobs09.cwp.20.

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Honda, Morihiro. "Atmospheric Neutrino Flux Calculation with NRLMSISE-00 Atmosphere Model and New Cosmic Ray Observations." In Proceedings of the 10th International Workshop on Neutrino-Nucleus Interactions in Few-GeV Region (NuInt15). Journal of the Physical Society of Japan, 2016. http://dx.doi.org/10.7566/jpscp.12.010008.

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Kokourov, Victor D., Galina V. Vergasova, and Edward S. Kazimirovsky. "The role of planetary waves in the atmosphere-ionosphere interactions." In SPIE Proceedings, edited by Gennadii G. Matvienko and Vladimir P. Lukin. SPIE, 2004. http://dx.doi.org/10.1117/12.606358.

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Reports on the topic "Atmosphere interactions"

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Stanley, Rachel H. R., Thomas Thomas, Yuan Gao, Cassandra Gaston, David Ho, David Kieber, Kate Mackey, et al. US SOLAS Science Report. Woods Hole Oceanographic Institution, December 2021. http://dx.doi.org/10.1575/1912/27821.

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Abstract:
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 activities, facilitate interactions among atmospheric and ocean scientists, and strengthen US contributions to international SOLAS. In October 2019, with support from OCB, the OAIC convened an open community workshop, Ocean-Atmosphere Interactions: Scoping directions for new research with the goal of fostering new collaborations and identifying knowledge gaps and high-priority science questions to formulate a US SOLAS Science Plan. Based on presentations and discussions at the workshop, the OAIC and workshop participants have developed this US SOLAS Science Plan. The first part of the workshop and this Science Plan were purposefully designed around the five themes of the SOLAS Decadal Science Plan (2015-2025) (Brévière et al., 2016) to provide a common set of research priorities and ensure a more cohesive US contribution to international SOLAS.
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Jakubiak, Bogumil, Teddy Holt, Richard Hodur, Maciej Szpindler, and Leszek Herman-Izycki. Implementation of Modeling the Land-Surface/Atmosphere Interactions to Mesoscale Model COAMPS. Fort Belvoir, VA: Defense Technical Information Center, September 2010. http://dx.doi.org/10.21236/ada541836.

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Jakubiak, Bogumil, Richard Hodur, and Leszek Herman-Izycki. Implementation of Modeling the Land-Surface/Atmosphere Interactions to Mesoscale Model COAMPS. Fort Belvoir, VA: Defense Technical Information Center, September 2012. http://dx.doi.org/10.21236/ada574482.

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Jakubiak, Bogumil, Teddy Holt, Richard Hodur, Maciej Szpindler, and Leszek Herman-Izycki. Implementation of Modeling the Land-Surface/Atmosphere Interactions to Mesoscale Model COAMPS. Fort Belvoir, VA: Defense Technical Information Center, September 2011. http://dx.doi.org/10.21236/ada557104.

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Denning, Scott. Multi-Scale Land-Atmosphere Interactions: Modeling Convective Processes from Plants to Planet. Office of Scientific and Technical Information (OSTI), February 2021. http://dx.doi.org/10.2172/1766315.

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Randall, D. A., and T. G. Jensen. Clouds and ocean-atmosphere interactions. Final report, September 15, 1992--September 14, 1995. Office of Scientific and Technical Information (OSTI), October 1995. http://dx.doi.org/10.2172/132693.

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Colle, Brian A. An Investigation of Terrain-Atmosphere-Ocean Interactions Along the Coastal Regions of North America. Fort Belvoir, VA: Defense Technical Information Center, August 2002. http://dx.doi.org/10.21236/ada627714.

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Colle, Brian A. An Investigation of Terrain-Atmosphere-Ocean Interactions Along the Coastal Regions of North America. Fort Belvoir, VA: Defense Technical Information Center, September 2003. http://dx.doi.org/10.21236/ada629741.

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Colle, Brian A. An Investigation of Terrain-Atmosphere-Ocean Interactions Along the Coastal Regions of North America. Fort Belvoir, VA: Defense Technical Information Center, September 2001. http://dx.doi.org/10.21236/ada625765.

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Brasseur, James G. A HPC “Cyber Wind Facility” Incorporating Fully-Coupled CFD/CSD for Turbine-Platform-Wake Interactions with the Atmosphere and Ocean. Office of Scientific and Technical Information (OSTI), May 2017. http://dx.doi.org/10.2172/1355906.

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