Gotowa bibliografia na temat „Formation des masses d’eau”
Utwórz poprawne odniesienie w stylach APA, MLA, Chicago, Harvard i wielu innych
Spis treści
Zobacz listy aktualnych artykułów, książek, rozpraw, streszczeń i innych źródeł naukowych na temat „Formation des masses d’eau”.
Przycisk „Dodaj do bibliografii” jest dostępny obok każdej pracy w bibliografii. Użyj go – a my automatycznie utworzymy odniesienie bibliograficzne do wybranej pracy w stylu cytowania, którego potrzebujesz: APA, MLA, Harvard, Chicago, Vancouver itp.
Możesz również pobrać pełny tekst publikacji naukowej w formacie „.pdf” i przeczytać adnotację do pracy online, jeśli odpowiednie parametry są dostępne w metadanych.
Artykuły w czasopismach na temat "Formation des masses d’eau"
PIEL, S., J. PEROT, C. RODIQ i F. NAULEAU. "Modélisation cinétique de l’évolution des trihalométhanes à partir de l’absorbance UV 254 nm après chloration sur un réseau d’eau potable". Techniques Sciences Méthodes, nr 4 (20.04.2020): 21–30. http://dx.doi.org/10.36904/tsm/202004021.
Pełny tekst źródłaGirineza, YN, PA Ba, C. Coundoul, AL Diop, M. Diouf, RAM Ndiaye i CD Niang. "C84: Lipome géant infiltrant de la cuisse avec souffrance vasculaire : A propos d’un cas". African Journal of Oncology 2, nr 1 Supplement (1.03.2022): S35. http://dx.doi.org/10.54266/ajo.2.1s.c84.jowl1393.
Pełny tekst źródłaGalbraith, Peter S., Daniel Bourgault i Mélany Belzile. "Circulation et renouvellement des masses d’eau du fjord du Saguenay". Océanographie 142, nr 2 (5.06.2018): 36–46. http://dx.doi.org/10.7202/1047147ar.
Pełny tekst źródłaROUSSEL, Jean-Marc, Gaétan POTTIER, Didier AZAM, Régis VIGOUROUX, Frédéric MARCHAND, Nicolas BARGIER, Marie NEVOUX i in. "Inventaire de biodiversité des poissons et crustacés d’eau douce par pêche à l’électricité en petits cours d’eau tropicaux : réglages, efficacité et recommandations". Sciences Eaux & Territoires, nr 42 (29.01.2023): 55–60. http://dx.doi.org/10.20870/revue-set.2023.42.7268.
Pełny tekst źródłaNégrel, P., S. Roy, E. Petelet-Giraud, A. Brenot, R. Millot, P. Dutartre i I. Fournier. "Les outils de diagraphie chimique pour la caractérisation des masses d’eau". Techniques Sciences Méthodes, nr 11 (2008): 29–46. http://dx.doi.org/10.1051/tsm/200811029.
Pełny tekst źródłaSanchez, W., i J. M. Porcher. "Utilisation des biomarqueurs pour la caractérisation de l’état écotoxicologique des masses d’eau". Techniques Sciences Méthodes, nr 5 (2009): 29–38. http://dx.doi.org/10.1051/tsm/200905029.
Pełny tekst źródłaViglino, Liza, i Émilien Pelletier. "Butylétains dans les eaux du fjord du Saguenay (Canada) : menace pour l’écosystème d’un milieu semi-fermé ?" Revue des sciences de l'eau 19, nr 1 (21.02.2006): 11–22. http://dx.doi.org/10.7202/012260ar.
Pełny tekst źródłaAdour Garonne, Agence de l’eau. "Transcription des guides européens pour l’analyse économique des masses d’eau fortement modifiées. Essai d’application à l’hydroélectricité". Techniques Sciences Méthodes, nr 2 (2007): 60–67. http://dx.doi.org/10.1051/tsm/200702060.
Pełny tekst źródłaDournel, Sylvain, i Bertrand Sajaloli. "Les milieux fluviaux et humides en ville, du déni à la reconnaissance de paysages urbains historiques". Articles 41, nr 1 (31.01.2013): 5–21. http://dx.doi.org/10.7202/1013761ar.
Pełny tekst źródłaRapin, Anne, Marion Rabiet, Malgorzata Grybos, Brice Mourier, Alexis Fay, Tim Kestens i Véronique Deluchat. "Distribution spatiale et mobilité du phosphore sédimentaire dans une retenue hydroélectrique". Revue des sciences de l’eau 30, nr 1 (8.06.2017): 71–76. http://dx.doi.org/10.7202/1040066ar.
Pełny tekst źródłaRozprawy doktorskie na temat "Formation des masses d’eau"
Akhoudas, Camille. "Un nouveau regard sur la dynamique de l’océan Austral et ses interactions avec la cryosphère révélé par une approche isotopique". Electronic Thesis or Diss., Sorbonne université, 2020. http://www.theses.fr/2020SORUS464.
Pełny tekst źródłaThe Southern Ocean is a key component in global ocean circulation and the Earth's climate system. Despite the increase of in situ observations in this remote region since the 1990s (notably with the « satellite era » and major international observation programs such as WOCE, CLIVAR, GO-SHIP, or ARGO), this immense ocean remains largely unknown. However, it is essential to observe and understand the mechanisms of its dynamics as well as its variability with the aim to predict the future evolution of the climate system. In particular, one important characteristic of the Southern Ocean is that it is one of the main sites of deep ocean ventilation, which allows redistribution and sequestration of heat, freshwater, carbon, oxygen, and nutrients. This ventilation process is mainly associated with a vertical circulation connecting the ocean surface to the abyss, fueled by intense interactions and exchanges of energy and buoyancy fluxes between atmosphere, ocean and cryosphere. In this thesis, I apprehend some aspects of the Southern Ocean dynamics by providing a mechanistic view of large-scale circulation and its ongoing changes. The approach I use throughout this thesis is based on observations of stable water isotopes, a passive tracer commonly used in a large number of earth science disciplines, but until recently only sparsely used in physical oceanography. Stable water isotopes constitute a robust tool which, as a tracer of the origin of water, help to better characterize the different components of the hydrological cycle as well as its evolution. In particular, the isotopic composition of seawater represents an important imprint of water masses, containing information on the conditions of their formation and their evolution. In this thesis, beyond the important methodological work at sea and in the laboratory for the sampling, analysis and calibration of isotopic measurements, I use the stable water isotopes in combination with other more conventional tracers to apprehend, with a new perspective, the questions of the role of interactions between the Southern Ocean and the Antarctic Ice Sheet in large-scale circulation, the signature of surface waters in the abyss, or even the impact of changes in atmospheric or cryosphere regimes on the surface ocean. Beyond the only use of stable water isotopes, original approaches have allowed me to document melting and refreezing of one of the largest ice shelves in the world, which influences the characteristics of the dense waters, precursors of abyssal waters produced in the Weddell Sea. My results also reveal the proportion of these dense waters in bottom water formation in the Atlantic sector of the Southern Ocean. We detail the processes that lead to the formation of bottom waters and with this new insight, we demonstrate that past estimates of bottom water production, in apparent contradiction, were actually focusing on different processes. Finally, I propose to quantify the changes in freshwater inputs over the past three decades that influence the trends in surface properties in the Indian sector of the Southern Ocean. The results demonstrate that changes in the precipitation regime explain changes in the surface ocean characteristics impacting stratification with consequences for large-scale water mass formation and overturning circulation in the Southern Ocean
Lekouch, Imad. "Production d’eau potable par condensation passive de l’humidité atmosphérique (rosée)". Paris 6, 2010. http://www.theses.fr/2010PA066638.
Pełny tekst źródłaPetit, Tillys. "Caractérisation de la circulation autour, au-dessus et à travers (via des zones de fracture) la dorsale de Reykjanes". Thesis, Brest, 2018. http://www.theses.fr/2018BRES0061/document.
Pełny tekst źródłaThe Reykjanes Ridge is a major topographic feature of the North-Atlantic Ocean that extends from Iceland to the Charlie Gibbs Fracture Zone. Located between the Iceland Basin and the Irminger Sea, the Reykjanes Ridge strongly influences the subpolar gyre circulation and is a gate toward the deep convection areas. However, the circulation and distribution across the Reykjanes Ridge has never been directly quantified such that the characterization of the connection between the Iceland Basin and the Irminger Sea is still incomplete. As part of the Reykjanes Ridge Experiment project, we were able to analyze the circulation around, above and across the Reykjanes Ridge. Mainly based on hydrographic sections along and perpendicular to the ridge axis, the aim of this PhD thesis was thus to characterize the 3-D circulation and properties of the flow along and across the Reykjanes Ridge.We started by accurately quantifying geostrophic transports across the sections, which led to improvements in the treatment of S-ADCP data. Across the Reykjanes Ridge, the intensity of the wesward branch of the subpolar gyre was estimated at21.9 + 2.5 Sv in June – July 2015 with intensifications at the Bight Fracture Zone (BFZ) and at 59 – 62°N. At the BFZ, overflow waters are influenced by the bathymetry such as their hydrological properties evolve as they cross the Reykjanes Ridge. Finally, both the bathymetry and the cyclonic horizontal circulation of the Iceland Basin regulate the evoluton of the along-ridge flows by blocking water masses, and thus shaping the water mass distribution over the Reykjanes Ridge. In addition to waters from the crossridge flow, the Irminger Current incorporates waters from the center of the Irminger Sea
Sheehan, Patrick D., i Josh A. Eisner. "Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626418.
Pełny tekst źródłaCsengeri, Timea. "Formation des étoiles massives : la recherche et l'étude des phases précoces". Paris 7, 2010. http://www.theses.fr/2010PA077243.
Pełny tekst źródłaThe formation of high-mass stars is one of the fondamental problems in today's astrophysics. During this thesis observational constraints are put on theoretical models describing the formation of high-mass stars. A significant part of the presented work is dedicated to high angular-resolution follow-up observations of high-mass star-forming sites in the Cygnus-X molecular complex, because it offers the opportunity to reach individual collapsing objects with current interferometers. The first part focuses on the fragmentation and kinematic properties of a sample of IR-quiet massive dense cores. These are found to be sub-fragmented into a few, high-mass protostars (Bontemps et al 2010). Dense gas tracers show that at small-scales supersonic, organized flows are present, which may converge to the central potential of the proto-cluster providing additional mass for star-formation processes. A similar finding is presented in the most massive part of the Cygnus-X complex associated with the DR21(OH) clump, which is a rich protocluster at its early stage of evolution. It shows hierarchical fragmentation and may lead to the birth of an even richer cluster, than the Orion Nebuli Cluster. The cold dense gas of this clump shows similarly high level of kinematic complexity in thé form of organized, small-scale converging flows. Altogether this indicates that dynamical processes may govern the formation and evolution of massive dense cores and the high-mass protostars within them. In a larger-scale study it is shown, that even on several parsec scales dynamical processes may play an important role in building-up massive structures (Schneider et al. 2010)
Prygiel, Émilie. "Impact des remises en suspension du sédiment liées au trafic fluvial en rivières canalisées sur l’état des masses d’eau : application au bassin Artois-Picardie". Thesis, Lille 1, 2013. http://www.theses.fr/2013LIL10110/document.
Pełny tekst źródłaRivers channelization and creation of linking channels to facilitate industrial development and trade have led to a strong historical pollution and artificialization of aquatic environments that are now subjected to good potential status objectives. Sediment resuspension by navigation, its impact on water quality and the achievement of status are the main concern of this thesis. Sediment and water chemical quality of three channels of Northern France have been studied: the Deûle River, the Sensée River (both navigated) and the Scarpe River (not navigated). The rivers have varying concentrations of P and ETM (overall Deûle ~ Scarpe > Sensée), which are generally well trapped with sulfides in sediments. Although the concentrations of dissolved ETM remain relatively low compared to the levels recorded in the sediment, they can sometimes exceed the environmental quality standards of the WFD. Lability of these ETM estimated by DGT is weak, even for Pb which is however significantly accumulated by caged gammarids deployed on the three sites. The navigation seems to play a limited role in the enrichment of the water column in dissolved metals and phosphorus, as well as the oxygenation of surface waters. Phytoplankton appears to have a greater influence on the evolution of these environments. Finally, the impact of navigation on the chemical quality of the water remains limited due to the peculiar geochemistry of the Artois-Picardie basin
Imara, Nia, Abraham Loeb, Benjamin D. Johnson, Charlie Conroy i Peter Behroozi. "A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures across Cosmic Time". IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627101.
Pełny tekst źródłaBhurtun, Pratima. "Dynamique de la qualité des masses d’eau dans le bassin Artois-Picardie : compréhension des mécanismes actuels et prévision des évolutions dans un contexte de changement climatique". Thesis, Lille 1, 2018. http://www.theses.fr/2018LIL1R055.
Pełny tekst źródłaThe River Selle is a non-channelised stream in the Artois-Picardy basin and is considered as a priority waterbody by the Artois-Picardy Water Agency. The aim of this work was to study the spatio-temporal behaviour of several substances at different time scales, ranging from low-frequency (grab sampling, passive samplers) to high-frequency monitoring. More specifically, tracers of pollution reflecting urban, agricultural and industrial contamination (nitrates, phosphates, trace metal elements, pesticides, pharmaceutical residues, dissolved organic matter) were investigated. We confirmed that the River Selle is mainly fed by a nitrate-rich groundwater. Besides, the nitrates and atrazine concentrations in the river water were similar to those found in the groundwater. At the upstream of the river, the land-use is mainly dominated by agriculture whereas most of the urban islets are located at the downstream of the river. Consequently, during dry weather, ultra-trace concentrations of some pesticides and pharmaceutical residues were recorded and phosphate levels often exceeded 0.2 mg L-1. Due to the minor flow input of the wastewater treatment plants into the river, metallic contamination in the River Selle (particularly Gd and Zn) is quite low despite the high concentrations measured in wastewater effluents. Water quality issues during storm events were identified by high-frequency monitoring. Significant but time-limited peaks in phosphorus and organic carbon were observed, while nitrates were diluted. The composition of dissolved organic matter was studied by fluorescence spectroscopy. The spectral signature of different types of water (groundwater, surface water and wastewater effluents) was characterised as well as the origins of this organic matter (autochtonous vs allochthonous). Finally, these results enable to discuss qualitatively the future effects of climate change at a regional scale on the evolution of the water quality of the River Selle
Lannier, Justine. "Formation des planètes géantes autour des étoiles de faibles masses : contraintes observationnelles en imagerie (optique adaptative)". Thesis, Université Grenoble Alpes (ComUE), 2016. http://www.theses.fr/2016GREAY041/document.
Pełny tekst źródłaStudying exoplanets, and in particular gaseous giant planets, is a new field of modern astrophysics. Understanding how the giant planets form, dynamically evolve, evolve with time, and have an impact on potential other planets within a stellar system are part of the biggest challenges of this science. The development of the most efficient observational technics and optimal analysis tools have been necessary to bring answers to these problematics. This is the context in which I realized my PhD thesis. I present in this manuscript the three projects that I led during these last three years.First, I studied the occurrence rate of the giant planets that orbit around M dwarfs. To realize this statistical study, I used NaCo data from two surveys. The first survey was composed of M dwarfs, the second was made of AF stars that were already studied by members of our team. I developed a Monte Carlo code, and used the contrapositive logic to lead a comparative analysis of these two surveys. I also associated stellar to planet mass ratios to planetary formation scenarios. My conclusions are that giant planets can more easily be formed by core accretion around AF stars than around M dwarfs, for separations between 8 and 400 astronomical units. Wide-orbit giant planets are rare whatever the stellar mass (basically <20%).Then, I developed a statistical tool that combines radial velocity and direct imaging data of specific stars, to better constrain the giant planet population at all separations. The code that I wrote is based on a Monte Carlo generation of synthetic planet populations. I applied this code on radial velocity and direct imaging data from young and nearby stars: AUMic, ßPictoris, HD113337, and HD95086. The future applications will be numerous thanks to the increase of the time baseline of radial velocity data and thanks to new high contrast and high resolution instruments able to probe shorter regions.These first two projects have allowed me to understand how to reduce and analyse data, and to develop statistical tools useful for my last project. This last project consists of observing, reducing and analyzing radial velocity and direct imaging data of a sample of K5-M5 young and nearby dwarfs. This project will bring strong constraints on the gaseous giant planet population that orbits around low mass stars, from short to wider separations
Guilyardi, Eric. "Role de la physique oceanique sur la formation/consommation des masses d'eau dans un modele couple ocean-atmosphere". Toulouse 3, 1997. http://www.theses.fr/1997TOU30278.
Pełny tekst źródłaKsiążki na temat "Formation des masses d’eau"
Prusti, Timo Juhani. Infrared studies of low mass formation. [Groningen, Netherlands]: Rijksuniversiteit Groningen, 1992.
Znajdź pełny tekst źródłaK, Dupree Andrea, Lago, M. T. V. T. i North Atlantic Treaty Organization. Scientific Affairs Division., red. Formation and evolution of low mass stars. Dordrecht: Kluwer Academic Publishers, 1988.
Znajdź pełny tekst źródłaMauritzen, Cecilie. A study of the large scale circulation and water mass formation in the Nordic Seas and the Arctic Ocean. [Wood Hole, Mass: Woods Hole Oceanographic Institution, 1994.
Znajdź pełny tekst źródłaFilimonova, Mariya. The Press becomes Power: Political Discussions on the Pages of the US Periodical Press in the Late 18th Century. ru: INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1213788.
Pełny tekst źródłaCappellari, Michele, i Stéphane Courteau. Galaxy Masses As Constraints of Formation Models (IAU S311). Cambridge University Press, 2015.
Znajdź pełny tekst źródła(Editor), A. K. Dupree, i Maria Teresa Vaz Torrão Lago (Editor), red. Formation and Evolution of Low Mass Stars (NATO Science Series C:). Springer, 2007.
Znajdź pełny tekst źródłaLancellotti, Patrizio, i Bernard Cosyns. Cardiac Source of Embolism (SOE) and Cardiac Masses. Oxford University Press, 2016. http://dx.doi.org/10.1093/med/9780198713623.003.0014.
Pełny tekst źródłaGoodin, Robert E., i Kai Spiekermann. Factionalism. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198823452.003.0014.
Pełny tekst źródłaSchrijver, Karel. The Worlds of Exoplanets. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198799894.003.0009.
Pełny tekst źródłaJha, Mithilesh Kumar. Language Politics and Public Sphere in North India. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780199479344.001.0001.
Pełny tekst źródłaCzęści książek na temat "Formation des masses d’eau"
Staroszczyk, Ryszard. "Formation and Types of Natural Ice Masses". W GeoPlanet: Earth and Planetary Sciences, 7–19. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-030-03038-4_2.
Pełny tekst źródłaBergin, Edwin A., i Jonathan P. Williams. "The Determination of Protoplanetary Disk Masses". W Formation, Evolution, and Dynamics of Young Solar Systems, 1–37. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-60609-5_1.
Pełny tekst źródłaMiddleman, Bruce, i Rob Earle. "Development of a Conceptual Groundwater Recovery System in a Fractured Bedrock Aquifer: A Case Study from the Wissahickon Formation". W Remediation in Rock Masses, 68–82. Reston, VA: American Society of Civil Engineers, 2000. http://dx.doi.org/10.1061/9780784400159.ch06.
Pełny tekst źródłaWuchterl, Günther. "Giant Planet Formation and the Masses of Extrasolar Planets". W Science with the VLT Interferometer, 64–71. Berlin, Heidelberg: Springer Berlin Heidelberg, 1997. http://dx.doi.org/10.1007/978-3-540-69398-7_6.
Pełny tekst źródłaThronson, Harley A. "No More Heterodyne Blues: Gas Masses From Millimeter and Sub-Millimeter Continuum Photometry". W Galactic and Extragalactic Star Formation, 621–26. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2973-9_40.
Pełny tekst źródłaJames, Phil. "Nearby Galaxies with UKIRT: Uncovering Star Formation, Structure and Stellar Masses". W Thirty Years of Astronomical Discovery with UKIRT, 213–27. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7432-2_20.
Pełny tekst źródłaSogacheva, L., L. Saukkonen, Miikka Dal Maso i Markku Kulmala. "Aerosol Particle Formation in Different Types of Air Masses in Hyytiälä, Southern Finland". W Nucleation and Atmospheric Aerosols, 591–95. Dordrecht: Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-6475-3_117.
Pełny tekst źródłaZerkal, O. V., E. V. Kalinin i L. L. Panasyan. "The Formation and Distribution of Stress Concentration Zones in Heterogeneous Rock Masses with Slopes". W Engineering Geology for Society and Territory - Volume 2, 1251–54. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-09057-3_219.
Pełny tekst źródłaMarsh, David J. E., i Sebastian Hoof. "Astrophysical Searches and Constraints". W The Search for Ultralight Bosonic Dark Matter, 73–122. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-95852-7_3.
Pełny tekst źródłaNakano, Takenori. "The Formation of Planets Around Stars of Various Masses and the Origin and the Evolution of Circumstellar Dust Clouds". W Star Forming Regions, 301–13. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_90.
Pełny tekst źródłaStreszczenia konferencji na temat "Formation des masses d’eau"
Denney, Kelly. "Measuring black hole masses at high redshift". W Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.169.0050.
Pełny tekst źródłaPeterson, Bradley, i Catherine Grier. "Masses of Black Holes in Active Galactic Nuclei". W Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.169.0030.
Pełny tekst źródłaIshikawa, K., Y. Tobita, Takuma Suda, Takaya Nozawa, Akira Ohnishi, Kiyoshi Kato, Masayuki Y. Fujimoto, Toshitaka Kajino i Shigeru Kubono. "Neutrino Masses and Mixing". W ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System. AIP, 2008. http://dx.doi.org/10.1063/1.2943594.
Pełny tekst źródłaManko, A. V., i E. A. Muraveva. "Fracture mechanics of fractured rock masses and verification of rheological calculation models". W CONSTRUCTION: THE FORMATION OF LIVING ENVIRONMENT: FORM-2022. AIP Publishing, 2023. http://dx.doi.org/10.1063/5.0144320.
Pełny tekst źródłaHerdiana, Hanifah Hilda, I. Gde Budi Indrawan i Hendy Setiawan. "Excavation method of rock masses at the tunnel 10 Jakarta - Bandung high-speed railway construction". W CONSTRUCTION: THE FORMATION OF LIVING ENVIRONMENT: FORM-2022. AIP Publishing, 2023. http://dx.doi.org/10.1063/5.0130057.
Pełny tekst źródłavan der Kruit, P. C., Victor P. Debattista i C. C. Popescu. "HI Velocity Dispersions and Flaring: Disk Masses and the Shape of Dark Matter Halos". W HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458541.
Pełny tekst źródłaFitriyantina, Laela, Doni Prakasa Eka Putra i I. Gde Budi Indrawan. "Rock mass quality determination of weak rock masses for design of Narogong diversion tunnel in West Java, Indonesia". W CONSTRUCTION: THE FORMATION OF LIVING ENVIRONMENT: FORM-2022. AIP Publishing, 2023. http://dx.doi.org/10.1063/5.0130027.
Pełny tekst źródłaWijaya, Brilyan J., I. Wayan Warmada i I. Gde B. Indrawan. "Correlation between GSI, RMR, and Q systems of rock masses at the construction site of spillway tunnel at Meninting Dam". W CONSTRUCTION: THE FORMATION OF LIVING ENVIRONMENT: FORM-2022. AIP Publishing, 2023. http://dx.doi.org/10.1063/5.0129879.
Pełny tekst źródłaWang, Jianqiang, i Zhiqi Yu. "Notice of Retraction: The Formation and Analysis of the Earth Gravitation Model Based on Point Masses". W 2010 2nd International Conference on Information Engineering and Computer Science (ICIECS). IEEE, 2010. http://dx.doi.org/10.1109/iciecs.2010.5678404.
Pełny tekst źródłaLakeram, Scott, J. Bret Bennington i Dennis Radcliffe. "GEOCHEMICAL AND SEM ANALYSES REVEAL NO CONCLUSIVE EVIDENCE THAT MORRISON FORMATION SILICIFIED MASSES ARE HERBIVORE COPROLITES". W GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-303914.
Pełny tekst źródłaRaporty organizacyjne na temat "Formation des masses d’eau"
Gorbov, Alexander. Converted fuels for smart home infrastructure. Part 1 - Converted types of innovative fuels and fuel mixtures. Intellectual Archive, czerwiec 2023. http://dx.doi.org/10.32370/iaj.2854.
Pełny tekst źródłaRamsey, Andree L., Heather H. Furey i Amy S. Bower. Overturning of the Subpolar North Atlantic Program (OSNAP): RAFOS Float Data Report June 2014 - January 2019. Woods Hole Oceanographic Institution, grudzień 2022. http://dx.doi.org/10.1575/1912/29540.
Pełny tekst źródłaDemchenko, Dmytro. DEMASSIFICATION OF SOCIAL PROCESSES IN THE CONTEXT OF DIGITAL COMMUNICATION (TO THE PROBLEM OF THE DICHOTOMY OF “ELITE-MASS” AS A POLITICAL COMMUNICATION PARADOX). Ivan Franko National University of Lviv, marzec 2024. http://dx.doi.org/10.30970/vjo.2024.54-55.12171.
Pełny tekst źródła