Relevant bibliographies by topics / "This Way for the Gas

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic '"This Way for the Gas'

Author: Grafiati
Published: 24 April 2022

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Journal articles on the topic ""This Way for the Gas"

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Tirelli, Giulio. "Natural Gas Propulsion -The Greenest Way." Journal of The Japan Institute of Marine Engineering 44, no. 6 (2009): 870–75. http://dx.doi.org/10.5988/jime.44.870.

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Plank, Raymond. "Changing the way we market gas." Natural Gas 12, no. 4 (2007): 11–14. http://dx.doi.org/10.1002/gas.3410120404.

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Carmichael, Jim. "More gas from Canada on way." Natural Gas 14, no. 1 (2007): 19–22. http://dx.doi.org/10.1002/gas.3410140105.

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Englmaier, Peter, and Ortwin Gerhard. "Milky Way Gas Dynamics." Celestial Mechanics and Dynamical Astronomy 94, no. 4 (2006): 369–79. http://dx.doi.org/10.1007/s10569-006-9003-3.

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Willett, Mark M. "On the Way to More Electronic Data Interchange." Natural Gas 5, no. 11 (2008): 14–16. http://dx.doi.org/10.1002/gas.3410051104.

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Grenier, Edward J. "Tennessee GSR: The way out of the wilderness." Natural Gas 13, no. 11 (2007): 27–29. http://dx.doi.org/10.1002/gas.3410131108.

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Helfer, Tamara T., and Leo Blitz. "Dense Gas in the Milky Way." Astrophysical Journal 478, no. 1 (1997): 233–45. http://dx.doi.org/10.1086/303774.

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Nasoudi-Shoar, S., P. Richter, and K. S. de Boer. "Density variations in Milky Way gas." EAS Publications Series 56 (2012): 77–80. http://dx.doi.org/10.1051/eas/1256009.

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Muraki, H., S. Kondo, and S. Matsumoto. "3-Way exhaust gas treatment catalysts." Zeolites 11, no. 2 (1991): 196. http://dx.doi.org/10.1016/0144-2449(91)80438-6.

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Buccigross, James H. "Gas industry leads way in adopting internet for electronic commerce." Natural Gas 16, no. 12 (2007): 15–20. http://dx.doi.org/10.1002/gas.3410161204.

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Dissertations / Theses on the topic ""This Way for the Gas"

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Tobin, Myreene. "Leading the way in oil and gas sustainable development." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/MQ59489.pdf.

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Deul, Erik Ronald. "Interstellar dust and gas in the Milky Way and M33." Leiden : Sterrewacht Leiden, 1988. http://catalog.hathitrust.org/api/volumes/oclc/18547726.html.

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Pachler, Klaus, Thomas Frank, and Klaus Bernert. "Simulation of Unsteady Gas-Particle Flows including Two-way and Four-way Coupling on a MIMD Computer Architectur." Universitätsbibliothek Chemnitz, 2002. http://nbn-resolving.de/urn:nbn:de:bsz:ch1-200200352.

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The transport or the separation of solid particles or droplets suspended in a fluid flow is a common task in mechanical and process engineering. To improve machinery and physical processes (e.g. for coal combustion, reduction of NO_x and soot) an optimization of complex phenomena by simulation applying the fundamental conservation equations is required. Fluid-particle flows are characterized by the ratio of density of the two phases gamma=rho_P/rho_F, by the Stokes number St=tau_P/tau_F and by the loading in terms of void and mass fraction. Those numbers (Stokes number, gamma) define the flow regime and which relevant forces are acting on the particle. Dependent on the geometrical configuration the particle-wall interaction might have a heavy impact on the mean flow structure. The occurrence of particle-particle collisions becomes also more and more important with the increase of the local void fraction of the particulate phase. With increase of the particle loading the interaction with the fluid phase can not been neglected and 2-way or even 4-way coupling between the continous and disperse phases has to be taken into account. For dilute to moderate dense particle flows the Euler-Lagrange method is capable to resolve the main flow mechanism. An accurate computation needs unfortunately a high number of numerical particles (1,...,10^7) to get the reliable statistics for the underlying modelling correlations. Due to the fact that a Lagrangian algorithm cannot be vectorized for complex meshes the only way to finish those simulations in a reasonable time is the parallization applying the message passing paradigma. Frank et al. describes the basic ideas for a parallel Eulererian-Lagrangian solver, which uses multigrid for acceleration of the flow equations. The performance figures are quite good, though only steady problems are tackled. The presented paper is aimed to the numerical prediction of time-dependend fluid-particle flows using the simultanous particle tracking approach based on the Eulerian-Lagrangian and the particle-source-in-cell (PSI-Cell) approach. It is shown in the paper that for the unsteady flow prediction efficiency and load balancing of the parallel numerical simulation is an even more pronounced problem in comparison with the steady flow calculations, because the time steps for the time integration along one particle trajectory are very small per one time step of fluid flow integration and so the floating point workload on a single processor node is usualy rather low. Much time is spent for communication and waiting time of the processors, because for cold flow particle convection not very extensive calculations are necessary. One remedy might be a highspeed switch like Myrinet or Dolphin PCI/SCI (500 MByte/s), which could balance the relative high floating point performance of INTEL PIII processors and the weak capacity of the Fast-Ethernet communication network (100 Mbit/s) of the Chemnitz Linux Cluster (CLIC) used for the presented calculations. Corresponding to the discussed examples calculation times and parallel performance will be presented. Another point is the communication of many small packages, which should be summed up to bigger messages, because each message requires a startup time independently of its size. Summarising the potential of such a parallel algorithm, it will be shown that a Beowulf-type cluster computer is a highly competitve alternative to the classical main frame computer for the investigated Eulerian-Lagrangian simultanous particle tracking approach.
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Strömgren, Tobias. "Modelling of turbulent gas-particle flow." Licentiate thesis, KTH, Mechanics, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-4639.

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<p>An Eulerian-Eulerian model for dilute gas-particle turbulent flows is</p><p>developed for engineering applications. The aim is to understand the effect of particles on turbulent flows. The model is implemented in a finite element code which is used to perform numerical simulations. The feedback from the particles on the turbulence and the mean flow of the gas in a vertical channel flow is studied. In particular, the influence of the particle response time and particle volume fraction on the preferential concentration of the particles near the walls, caused by the turbophoretic effect is explored. The study shows that the particle feedback decreases the accumulation of particles on the walls. It is also found that even a low particle volume fraction can have a significant impact on the turbulence and the mean flow of the gas. A model for the particle fluctuating velocity in turbulent gas-particle flow is derived using a set of stochastic differential</p><p>equations. Particle-particle collisions were taken into account. The model shows that the particle fluctuating velocity increases with increasing particle-particle collisions and that increasing particle response times decrease the fluctuating velocity.</p>
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Yiallourides, Constantinos. "Joint development of oil and gas resources : the way forward in disputed waters." Thesis, University of Aberdeen, 2017. http://digitool.abdn.ac.uk:80/webclient/DeliveryManager?pid=231747.

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The settlement of the maritime boundary disputes between China and Japan in the East China Sea, and between Greece and Turkey in the Aegean Sea, is politically deadlocked. While diplomatic settlement efforts have been ongoing for the past several decades, neither side in each case appears prepared to back down from its respective maritime claims. Bilateral consultations and negotiations have been unable to prevent occasional flare-ups and, as tensions remain significantly high, it may not be long before one of the not infrequent confrontations spirals out of control. The existing status quo in each case is unstable and does not favour either side, both from the perceptive of contaminating bilateral relations as a whole, but also to the extent that it holds hostage the multiple benefits that could otherwise be generated from the exploitation of the seabed energy resources in the contested waters. Indeed, while important discoveries of commercial hydrocarbon accumulations have been made, and in fact, some of them are currently being developed in the peripheries of the East China Sea and the Aegean, the full mineral potential of the contested areas remain unproven and unrealised due to the ongoing maritime and territorial conflicts. That being the case, the debate surrounding these two conflicts has progressed to the point where there is an urgent need for a meaningful discussion on finding a practical way forward. It is the purpose of the present thesis to address this need, first, by undertaking a detailed analysis of these disputes on the basis of the legal rules and principles of international law and; second, by critically evaluating possible institutional designs of interstate cooperation on the exploitation of offshore oil and gas resources in disputed areas. This thesis considers that because of the near-impossibility of settling the maritime and territorial disputes in the East China Sea and the Aegean, at least in the short term, and the remote possibility of meaningfully utilising the resources in the given areas while these conflicts persist, provisional interstate cooperation in the form of joint development constitutes the best alternative course of action for disputing states to coordinate the exploration and exploitation of resources without having resorted previously to boundary delimitation settlement. On the basis of the above analysis, this thesis discusses the prospect of realising joint development regimes in the East China Sea and the Aegean and their appropriate institutional design in the light of the legal, historical, political, and geographical characteristics of the disputes in question. The overall aim of the present study is to discern useful guidelines that can be used to inform and support diplomatic discussions on bilateral cooperation over disputed seabed energy resources by addressing three key objectives: - Better understanding of the longstanding East China Sea and Aegean maritime boundary disputes under the rules of the public international law of the sea, as developed to date having regard to international jurisprudence and state practice. - Conceptualisation and better understanding of the legal characteristics and functional benefits of joint development regimes. - Critical evaluation of variations in the design of joint development regimes having regard to successful or unsuccessful precedents in the practice of states.
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Pidopryhora, Yurii. "Extra-Planar HI in the Inner Milky Way." Ohio University / OhioLINK, 2006. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1162881965.

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Zeren, Zafer. "Lagrangian stochastic modeling of turbulent gas-solid flows with two-way coupling in homogeneous isotropic turbulence." Thesis, Toulouse, INPT, 2010. http://www.theses.fr/2010INPT0106/document.

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Dans ce travail de thèse, réalisé à l'IMFT, nous nous sommes intéressés aux écoulements turbulents diphasiques gaz-solides et plus particulièrement au phénomène de couplage inverse qui correspond à la modulation de la turbulence par la phase dispersée. Ce mécanisme est crucial pour les écoulements à forts chargements massiques. Dans cette thèse, nous avons considéré une turbulence homogène isotrope stationnaire sans gravité dans laquelle des particules sont suivies individuellement d'une façon Lagrangienne. La turbulence du fluide porteur est obtenue par des simulations directes (DNS). Les particules sont sphériques, rigides et d'une taille inférieure aux plus petites échelles de la turbulence. Leur densité est bien plus grande que la densité du fluide. Dans ce cadre, la force la plus importante agissant sur les particules est celle de traînée. Les interactions inter-particules ainsi que la gravité ne sont pas prises en compte. Pour modéliser ce type d'écoulement, une approche stochastique est utilisée pour laquelle l'accélération du fluide est modélisée par une équation de Langevin. L'originalité de ce travail est la prise en compte de l'effet de la modulation de la turbulence par un terme additionnel. Nous avons proposé deux modèles : une force de couplage moyenne qui est définie à partir des vitesses moyennes des phases, et une force instantanée qui est définie à l'aide du formalisme mésoscopique Eulérien. La fermeture des modèles s’appuie sur la fonction d’autocorrélation Lagrangienne et l’équation de transport de l’énergie cinétique. Les modèles sont testés en terme de prédiction de la vitesse de dérive et des corrélations fluide-particule. Les résultats montrent que le modèle moyen, plus simple, prend en compte les effets principaux du couplage inverse. Cependant, le problème de fermeture pratique est reporté sur la modélisation de l’échelle intégrale Lagrangienne et l’énergie cinétique de la turbulence du fluide vue par les particules<br>In this thesis, performed in IMFT, we are interested in the turbulent gas-solid flows and more specifically, in the phenomenon of turbulence modulation which is the modification of the structure of the turbulence due to the solid particles. This mechanism is crucial in flows with high particle mass-loadings. In this work, we considered a homogeneous isotropic turbulence without gravity kept stationary with stochastic type forcing. Discrete particles are tracked individually in Lagrangian manner. Turbulence of the carrier phase is obtained by using DNS. The particles are spherical, rigid and of a diameter smaller than the smallest scales of turbulence. Their density is very large in comparison to the density of the fluid. In this configuration the only force acting on the particles is the drag force. Volume fraction of particles is very small and inter-particle interactions are not considered. To model this type of flow, a stochastic approach is used where the fluid element accel- eration is modeled using stochastic Langevin equation. The originality in this work is an additional term in the stochastic equation which integrates the effect of the particles on the trajectory of fluid elements. To model this term, we proposed two types of modeling: a mean drag model which is defined using the mean velocities from the mean transport equations of the both phases and an instantaneous drag term which is written with the help of the Mesoscopic Eulerian Approach. The closure of the models is based on the Lagrangian auto- correlation function of the fluid velocity and on the transport equation of the fluid kinetic energies. The models are tested in terms of the fluid-particle correlations and fluid-particle turbulent drift velocity. The results show that the mean model, simple, takes into account the principal physical mechanism of turbulence modulation. However, practical closure problem is brought forward to the Lagrangian integral scale and the fluid kinetic energy of the fluid turbulence viewed by the particles
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Strömgren, Tobias. "Model predictions of turbulent gas-particle shear flows." Doctoral thesis, KTH, Mekanik, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-12135.

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A turbulent two-phase flow model using kinetic theory of granularflows for the particle phase is developed and implmented in afinite element code. The model can be used for engineeringapplications. However, in this thesis it is used to investigateturbulent gas-particle flows through numerical simulations.  The feedback from the particles on the turbulence and the meanflow of the gas in a vertical channel flow is studied. In particular,the influence of the particle response time, particle volumefraction and particle diameter on the preferential concentration ofthe particles near the walls, caused by the turbophoretic effect isexplored. The study shows that when particle feedback is includedthe accumulation of particles near the walls decreases. It is also foundthat even at low volume fractions particles can have a significant impacton the turbulence and the mean flow of the gas. The effect of particles on a developing turbulent vertical upward pipeflow is also studied. The development length is found to substantiallyincrease compared to an unladen flow. To understand what governs thedevelopment length a simple estimation was derived, showing that itincreases with decreasing particle diameters in accordance with themodel simulations. A model for the fluctuating particle velocity in turbulentgas-particle flow is derived using a set of stochastic differentialequations taking into account particle-particle collisions. Themodel shows that the particle fluctuating velocity increases whenparticle-particle collisions become more important and that increasingparticle response times reduces the fluctuating velocity. The modelcan also be used for an expansion of the deterministic model for theparticle kinetic energy.<br>QC20100726
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Canducci, Marco. "Adaptive-mesh refinement hydrodynamical simulations of cold gas clouds in the hot corona of the Milky Way." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/12832/.

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Le galassie star-forming, come la Via Lattea, hanno formato stelle durante tutta la propria vita (~ 12 Gyr). Tuttavia, tipicamente la massa di gas contenuta nel disco di tali galassie può sostenere la formazione stellare solo per pochi Gyr. Tale problema (gas-consumption dilemma) suggerisce la necessità di un continuo accrescimento di gas freddo da parte del disco della galassia ad un tasso di ~ 1 M_Sol /yr. Modelli teorici cosmologici e recenti osservazioni in banda X mostrano che tali galassie sono circondate da corone di gas caldo alla temperatura viriale (T ~ 10^6 K per la MW). Queste corone, se in grado di raffreddare, potrebbero sostenere il processo di formazione stellare agli attuali tassi osservati. Simulazioni idrodinamiche in 2D realizzate negli ultimi anni hanno mostrato che il gas coronale caldo può raffreddare efficientemente in seguito all’interazione con nubi di fontana galattica, processo sostenuto dalle esplosioni di supernove. La coda turbolenta, formatasi in seguito allo sviluppo di un'instabilità di Kelvin-Helmholtz, causa la diminuzione del tempo di cooling di parte del gas coronale e la sua condensazione. Questo gas condensato (10-20% della massa iniziale della nube) ricade sul disco alimentando la formazione stellare. In questa tesi estendiamo la trattazione della nube di fontana galattica ad una geometria 3D. I codici finora utilizzati, a griglia fissa, non permettono tale trattazione per via del proibitivo costo computazionale. Abbiamo quindi utilizzato ENZO, un codice a griglie adattive che raffina la risoluzione solo in zone soddisfacenti alcuni criteri. Abbiamo realizzato una serie di simulazioni idrodinamiche in 2D sia nel caso in cui il gas non possa raffreddare radiativamente sia nel caso contrario e per entrambi è stato individuato il criterio di raffinazione più performante. Tale criterio è stato utilizzato per una simulazione 3D, ricavando un valore per la condensazione quasi doppio rispetto alla trattazione precedente (~ 30%).
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Lucas, William. "Gas flow and star formation in the centre of the Milky Way : investigations with smoothed particle hydrodynamics." Thesis, University of St Andrews, 2015. http://hdl.handle.net/10023/6601.

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The centre of the Milky Way, commonly referred to as the Galactic Centre, is roughly that region within 500 pc of the central black hole, Sagittarius A*. Within the innermost parsec around the supermassive black hole Sagittarius A* are more than a hundred massive young stars whose orbits align to form one or possibly two discs. At about 100 pc is a ring containing more than ten million solar masses of molecular gas which could be the origin of some of the most massive star clusters in the Galaxy. I have performed a number of numerical simulations to help us understand how it is that these structures may have been formed. I firstly describe and test an improvement to the smoothed particle hydrodynamics code I used. This improves conservation of energy and momentum in certain situations such as in strong shocks from supernovae, which were to be included in a later chapter. The discs of massive stars around Sagittarius A* are believed to have been born there within fragmenting gaseous discs. This is problematic, as the formation of two stellar discs would require two gaseous counterparts. A method is described of forming multiple discs around a black hole from a single cloud's infall and subsequent tidal destruction. This is due to its prolate shape providing a naturally large distribution in the direction of the angular momentum vectors within the cloud. The resulting discs may then go on to form stars. Energetically, it would appear that a sequence of supernovae could potentially cause a giant molecular cloud to fall inwards towards the central black hole from an originally large orbit around the Galactic Centre. I simulate the impact on a giant molecular cloud of supernovae originating from a massive stellar cluster located a parsec away. Ultimately, the supernovae are found to have little effect. Finally, I simulate the formation of the dense ring of clouds observed in the Central Molec- ular Zone at a distance of about 100 pc from Sgr A*. Infalling gas is shown to be subject to such extreme tidal forces that a single cloud of gas is extended to form a long stream. The ribbon grows to the point that it self-intersects and forms a ring-like structure. Its complexity depends on the orbit of the original cloud. The position-velocity data is compared with observations, and similarities are noted.
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Books on the topic ""This Way for the Gas"

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Paving the way to natural gas vehicles. INFORM, 1993.

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Sonzogni, Marco. This way: Covering/uncovering Tadeusz Borowski's this way for the gas, ladies and gentlemen. Dunmore Pub., 2011.

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Deul, Erik Ronald. Interstellar dust and gas in the Milky Way and M33. Sterrewacht Leiden, 1988.

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Commission, United States Federal Energy Regulatory. An interstate natural gas facility on my land?: What do I need to know? Federal Energy Regulatory Commission, 2013.

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Region, United States Minerals Management Service Gulf of Mexico OCS. Destin Dome 56 unit development and production plan and right-of-way pipeline application: Draft environmental impact statement. The Region, 1999.

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Jackson, Neville. No end to the way. Corgi, 1985.

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To authorize the Secretary of the Interior to issue right-of-way permits for natural gas pipelines within the boundary of Great Smoky Mountains National Park: Report (to accompany H.R. 3380) (including cost estimate of the Congressional Budget Office). U.S. G.P.O., 2002.

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Lassell, Michael. The hard way. Masquerade Books, 1995.

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Mastbaum, Blair. Clay's Way. Alyson Books, 2004.

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Schwab, Rochelle H. In a family way. Orlando Place Press, 1995.

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Book chapters on the topic ""This Way for the Gas"

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Brutschin, Elina. "The Way Forward." In EU Gas Security Architecture. Palgrave Macmillan UK, 2016. http://dx.doi.org/10.1057/978-1-137-51150-8_6.

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Richter, Philipp. "Gas Accretion onto the Milky Way." In Gas Accretion onto Galaxies. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-52512-9_2.

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Carlberg, R. G. "Gas Dynamics and Disk-Galaxy Evolution." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_122.

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Pradhan, Sanjay Kumar. "The Way Forward." In India’s Quest for Energy Through Oil and Natural Gas. Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-5220-5_10.

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Van Woerden, Hugo, Ronald J. Allen, and W. Butler Burton. "Large-Scale Distribution and Motions of Gas." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_28.

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Lacey, Cedric G. "Heating of Stellar Disks by Massive Gas Clouds." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_95.

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Dickey, John M. "Small-Scale Structure and Motions in the Interstellar Gas." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_62.

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Johns, T. C., and A. H. Nelson. "3-Dimensional Particle Simulation of Vertical Oscillations in Gas Discs." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_98.

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Koyama, K., and Y. Maeda. "The Hot Gas in the Galactic Bulge." In Unsolved Problems of the Milky Way. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-1687-6_38.

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Sakamoto, S., T. Hasegawa, T. Handa, T. Oka, and M. Hayashi. "Physical Conditions of Molecular Gas in the Galaxy." In Unsolved Problems of the Milky Way. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-1687-6_72.

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Conference papers on the topic ""This Way for the Gas"

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Skaloud, D., R. Karavadi, and A. Matkienko. "Where Gas is Water - and Water is Gas." In EAGE Workshop on Detective Stories Behind Prospect Generation - Challenges and the Way Forward. European Association of Geoscientists & Engineers, 2009. http://dx.doi.org/10.3997/2214-4609.201404659.

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Daungkaew, Saifon, Go Fujisawa, Suchart Chokthanyawat, et al. "Is There A Better Way to Determine The Viscosity in Waxy Crudes?" In SPE Asia Pacific Oil and Gas Conference and Exhibition. Society of Petroleum Engineers, 2012. http://dx.doi.org/10.2118/159337-ms.

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Romanov, A. S., and E. F. Zolnikova. "Gas/Oil Reservoir Pressure Maintenance by Way of Gas Injection (Russian)." In SPE Russian Oil and Gas Technical Conference and Exhibition. Society of Petroleum Engineers, 2008. http://dx.doi.org/10.2118/117426-ru.

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Qutob, Hani Husien, and Horacio Ferreira. "The SURE way to underbalanced Drilling." In SPE Middle East Oil and Gas Show and Conference. Society of Petroleum Engineers, 2005. http://dx.doi.org/10.2118/93346-ms.

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Mckay, Wayne, and Jim Maddocks. "Acid Gas Dehydration - Is There a Better Way?" In Offshore Technology Conference. Offshore Technology Conference, 2012. http://dx.doi.org/10.4043/23549-ms.

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van der Wal, Jakob. "HSE, A Way Of Living." In SPE International Conference on Health, Safety, and Environment in Oil and Gas Exploration and Production. Society of Petroleum Engineers, 2008. http://dx.doi.org/10.2118/111881-ms.

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Simonin, Olivier, and Kyle D. Squires. "On Two-Way Coupling in Gas-Solid Turbulent Flows." In ASME/JSME 2003 4th Joint Fluids Summer Engineering Conference. ASMEDC, 2003. http://dx.doi.org/10.1115/fedsm2003-45739.

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An analysis of kinetic energy transfer in particle-laden turbulent flows is presented. The present study focuses on the subset in which dispersed-phase motion is restricted to particles in translation, particle diameters are smaller than the smallest lengthscales in the turbulent carrier flow, and the dispersed phase is present at negligible volume fraction. An analysis of the separate and exact two-fluid mean and turbulent kinetic energy transport equations shows that momentum exchange between the phases results in a transfer of kinetic energy from the mean to the fluctuating motion of the two-phase mixture. The source term accounting for fluid-particle coupling in the fluid turbulent kinetic energy equation is written as the sum of three parts, the first part representing the production of velocity fluctuations in the particle wake (“pseudo turbulence”), the second and third contributions — which act primarily on the larger scales of the fluid turbulent motion — representing a damping effect due to the turbulent fluctuation of the drag force and the effect of the transport of the particles by the fluid turbulence against their mean relative motion. A schematic representation of the energy transfers in particle-laden mixtures is also presented for the simplified systems under consideration, consistent with the separation of scales between perturbations introduced at the scale of the particle and the large, energy-containing scales of fluid turbulent motion. Implications of the energy transfers for ensemble-averaged modeling approaches are discussed, along with computational techniques that account for the back-effect of the particles on the flow using the point-force approximation. It is shown that the point-force approximation as typically implemented only accounts for the modulation of the large eddies, the contribution to wake production is not included, being implicitly assumed to be in local equilibrium with the corresponding viscous dissipation.
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Lu, Hsueh-Tsung, Yutao Qin, and Yogesh B. Gianchandani. "A Hybrid Three-Way Valve for Gas Chromatography Systems." In 2018 IEEE Sensors. IEEE, 2018. http://dx.doi.org/10.1109/icsens.2018.8589847.

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Stenning, David G., John P. Fitzpatrick, and Mark A. Trebble. "Floating CNG, A Simpler Way to Monetise Offshore Gas." In Offshore Technology Conference. Offshore Technology Conference, 2012. http://dx.doi.org/10.4043/23615-ms.

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Dame, T. M. "The distribution of neutral gas in the Milky Way." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.43985.

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Reports on the topic ""This Way for the Gas"

1

Fung, K. B., D. W. Fraser, and R. P. Gauthier. Application of Remote Sensing Data for Monitoring of Gas Pipeline Right-of-Way. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 1998. http://dx.doi.org/10.4095/219196.

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Sullivan, B. J., A. C. McGraw, and D. O. Johnson. Environmental aspects of rights-of-way for natural gas transmission pipelines: An updated bibliography: Final report, September 1987--June 1988. Office of Scientific and Technical Information (OSTI), 1988. http://dx.doi.org/10.2172/6211665.

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Takada, Yogo, Toshimasa Kotani, Kazuma Ito, Sang-kyu Kim, and Tomoyuki Wakisaka. Application of a Genetic Algorithm to the Numerical Analysis of Thermo-Fluid Flow and Catalytic Reaction in an Exhaust Gas Three-Way Catalyzer. SAE International, 2005. http://dx.doi.org/10.4271/2005-08-0487.

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Reppert, T., and J. Chiu. Heavy-Duty Waste Hauler with Chemically Correct Natural Gas Engine Diluted with EGR and Using a Three-Way Catalyst: Final Report, 24 February 2004 -- 23 February 2006. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/15020308.

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Boyer, Brian. Safeguards at Gas Centrifuge Enrichment Plants: Why is Iran a Threat? Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1136096.

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Lee, Ernest C. Sarin Nerve Gas: A Rationale for Vigilance Amidst War and Peace. Defense Technical Information Center, 2003. http://dx.doi.org/10.21236/ada415163.

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Margot Gerritsen. Industrial Compositional Streamline Simulation for Efficient and Accurate Prediction of Gas Injection and WAG Processes. Office of Scientific and Technical Information (OSTI), 2008. http://dx.doi.org/10.2172/950479.

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Miyamoto, Akira, and Chikako Ishiguro. The outlook for natural gas and LNG in China in the war against air pollution. Oxford Institute for Energy Studies, 2018. http://dx.doi.org/10.26889/9781784671242.

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Simon, James E., Uri M. Peiper, Gaines Miles, A. Hetzroni, Amos Mizrach, and Denys J. Charles. Electronic Sensing of Fruit Ripeness Based on Volatile Gas Emissions. United States Department of Agriculture, 1994. http://dx.doi.org/10.32747/1994.7568762.bard.

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An electronic sensory system for the evaluation of headspace volatiles was developed to determine fruit ripeness and quality. Two prototype systems were designed, constructed, and later modified. The first is an improved version of our original prototype electronic sniffer using a single head sensing unit for use as a single or paired unit placed on an individual fruit surface for applications in the field, lab, or industry. The second electronic sniffer utilizes a matrix of gas sensors, each selected for differential sensitivity to a range of volatile compounds. This system is more sophisticated as it uses multiple gas sensors, but was found to enhance the ability of the sniffer to classify fruit ripeness and quality relative to a single gas sensor. This second sniffer was designed and constructed for the sampling of fresh-cut or whole packs of fruits such as packaged strawberries and blueberries, and can serve as a prototype for research or commercial applications. Results demonstrate that electronic sensing of fruit ripeness based on aromatic volatile gas emissions can be used successfully with fresh frits. Aroma sensing was successful for classifying ripeness in muskmelons, including different cultivars, apples, blueberries, strawberries, and in a complimentary BARD project on tomatoes. This system compared favorably to the physicochemical measurements traditionally employed to assess fruit maturity. This nondestructive sensory system can detect the presence of physically damaged fruits and shows excellent application for use in quality assessment. Electronic sensors of the tin oxide type were evaluated for specificity toward a wide range of volatiles associated with fruit ripeness. Sensors were identified that detected a broad range of alcohols, aldehydes, esters, hydrocarbons, and volatile sulfur compounds, as well as individual volatiles associated with fruit ripening across a wide concentration range. Sensors are not compound specific, thus, the matrix of sensors coupled with discrimination analysis provides a fingerprint to identify the presence of compounds and to assess alterations in fresh products due to alterations in volatile emissions. Engineering developments led to the development of a system to compensate for temperature and relative humidity relative to on-line aroma sensing with melons for ripeness determination and to reduce response time, thus permitting the electronic sniffer to be used for monitoring both fresh and processed food products. The sniffer provides a fast, reliable and nondestructive tool to assess fruit ripeness and quality. We hope that our work will foster the introduction and utilization of this emerging technology into the agricultural and horticultural
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Echevarria, Antulio J., and II. An American Way of War or Way of Battle? Defense Technical Information Center, 2004. http://dx.doi.org/10.21236/ada426321.

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