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Articles de revues sur le sujet « Turbulence-Radiation interactions »

Auteur : Grafiati

Publié le 4 juin 2021

Mis à jour le 11 février 2022

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1

Kounalakis, M. E., J. P. Gore, and G. M. Faeth. "Turbulence/radiation interactions in nonpremixed hydrogen/air flames." Symposium (International) on Combustion 22, no. 1 (1989): 1281–90. http://dx.doi.org/10.1016/s0082-0784(89)80139-0.

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Mehta, R. S., M. F. Modest, and D. C. Haworth. "Radiation characteristics and turbulence–radiation interactions in sooting turbulent jet flames." Combustion Theory and Modelling 14, no. 1 (2010): 105–24. http://dx.doi.org/10.1080/13647831003660529.

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3

Consalvi, J. L., and F. Nmira. "Absorption turbulence-radiation interactions in sooting turbulent jet flames." Journal of Quantitative Spectroscopy and Radiative Transfer 201 (November 2017): 1–9. http://dx.doi.org/10.1016/j.jqsrt.2017.06.024.

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4

Nmira, Fatiha, Daria Burot, and Jean-Louis Consalvi. "Soot emission radiation–turbulence interactions in diffusion jet flames." Combustion Science and Technology 191, no. 1 (2018): 126–36. http://dx.doi.org/10.1080/00102202.2018.1452395.

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5

Mazumder, S., and M. F. Modest. "Turbulence-Radiation Interactions in Nonreactive Flow of Combustion Gases." Journal of Heat Transfer 121, no. 3 (1999): 726–29. http://dx.doi.org/10.1115/1.2826041.

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6

Silvestri, S., D. J. E. M. Roekaerts, and R. Pecnik. "Modelling turbulent heat flux accounting for Turbulence-Radiation Interactions." International Journal of Heat and Fluid Flow 89 (June 2021): 108728. http://dx.doi.org/10.1016/j.ijheatfluidflow.2020.108728.

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7

Li, Genong, and Michael F. Modest. "Importance of Turbulence-Radiation Interactions in Turbulent Diffusion Jet Flames." Journal of Heat Transfer 125, no. 5 (2003): 831–38. http://dx.doi.org/10.1115/1.1597621.

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Traditional modeling of radiative transfer in reacting flows has ignored turbulence-radiation interactions (TRI). Radiative fluxes, flux divergences and radiative properties have been based on mean temperature and concentration fields. However, both experimental and theoretical work have suggested that mean radiative quantities may differ significantly from those predictions based on the mean parameters because of their strongly nonlinear dependence on the temperature and concentration fields. The composition PDF method is able to consider many nonlinear interactions rigorously, and the method

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8

Curry, Judith A. "Interactions among Turbulence, Radiation and Microphysics in Arctic Stratus Clouds." Journal of the Atmospheric Sciences 43, no. 1 (1986): 90–106. http://dx.doi.org/10.1175/1520-0469(1986)043<0090:iatram>2.0.co;2.

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9

Gore, J. P., S. M. Jeng, and G. M. Faeth. "Spectral and Total Radiation Properties of Turbulent Hydrogen/Air Diffusion Flames." Journal of Heat Transfer 109, no. 1 (1987): 165–71. http://dx.doi.org/10.1115/1.3248038.

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A study of the structure and radiation properties of round turbulent hydrogen/air diffusion flames is described. Measurements were made of mean and fluctuating streamwise velocity, mean temperatures, species concentrations, spectral radiation intensities, and radiant heat fluxes. The measurements were used to evaluate predictions based on the laminar flamelet concept and narrow-band radiation models both ignoring (using mean properties) and considering (using a stochastic method) effects of turbulence/radiation interactions. State relationships found by correlating auxiliary measurements in la

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10

Kounalakis, M. E., J. P. Gore, and G. M. Faeth. "Mean and Fluctuating Radiation Properties of Nonpremixed Turbulent Carbon Monoxide/Air Flames." Journal of Heat Transfer 111, no. 4 (1989): 1021–30. http://dx.doi.org/10.1115/1.3250763.

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Mean and fluctuating spectral radiation intensities were measured for horizontal chordlike paths through turbulent nonpremixed carbon monoxide/air flames. Measurements in the 2700 nm radiation band of carbon dioxide revealed radiation fluctuations exceeding 50 percent in some locations even though mean radiation levels were not strongly influenced by turbulence/radiation interactions. Both time-independent and time-dependent stochastic simulations were developed to treat turbulence/radiation interactions as well as the temporal properties of flame radiation. The stochastic simulations were bas

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11

Modest, Michael F. "Multiscale Modeling of Turbulence, Radiation, and Combustion Interactions in Turbulent Flames." International Journal for Multiscale Computational Engineering 3, no. 1 (2005): 85–106. http://dx.doi.org/10.1615/intjmultcompeng.v3.i1.70.

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12

Silvestri, S., D. J. E. M. Roekaerts, and R. Pecnik. "Assessing turbulence-radiation interactions in turbulent flows of non-gray media." Journal of Quantitative Spectroscopy and Radiative Transfer 233 (August 2019): 134–48. http://dx.doi.org/10.1016/j.jqsrt.2019.05.018.

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13

Chan, S. H., and X. C. Pan. "A General Semicausal Stochastic Model for Turbulence/Radiation Interactions in Flames." Journal of Heat Transfer 119, no. 3 (1997): 509–16. http://dx.doi.org/10.1115/1.2824127.

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This paper presents a general two-dimensional non-stationary semicausal model for the simulation of mixture fraction, which improves our previous causal model. The proposed model includes not only the pre-correlation predictors (both in time space and geometric space) as well as the cross-correlation predictors, as in the causal model, but also post-correlation predictors. The latter makes possible the consideration of interactions of a scalar, such as mixture fraction, at a physical location with that of all its adjacent locations. It has also been shown that the complicated second-and higher

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14

Consalvi, J. L. "Influence of turbulence–radiation interactions in laboratory-scale methane pool fires." International Journal of Thermal Sciences 60 (October 2012): 122–30. http://dx.doi.org/10.1016/j.ijthermalsci.2012.05.013.

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15

Ren, Tao, Michael F. Modest, and Daniel C. Haworth. "Simulating turbulence–radiation interactions using a presumed probability density function method." International Journal of Heat and Mass Transfer 121 (June 2018): 911–23. http://dx.doi.org/10.1016/j.ijheatmasstransfer.2018.01.049.

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16

Lemos, L. D., F. R. Centeno, and F. H. R. França. "EFFECTS OF TURBULENCE-RADIATION INTERACTIONS IN A NON-PREMIXED TURBULENT METHANE-AIR FLAME." Revista de Engenharia Térmica 17, no. 1 (2018): 63. http://dx.doi.org/10.5380/reterm.v17i1.62260.

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This work studied a turbulent flame and analyzed the interaction between turbulence and radiation (TRI). The problem consists of a non-premixed turbulent methane flame surrounded by a low-velocity air coflow identified as Flame DLR-A. The steady laminar diffusion flamelet (SLDF) model is used to solve the chemical kinetics. To generate the flamelet library, turbulence-chemistry interaction is taken into account through previously assumed probability density functions (PDF) of mean scalars. Radiative heat flux is calculated with the discrete ordinates method, considering the Gray Gas model (GG)

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17

Gore, J. P., and G. M. Faeth. "Structure and Radiation Properties of Luminous Turbulent Acetylene/Air Diffusion Flames." Journal of Heat Transfer 110, no. 1 (1988): 173–81. http://dx.doi.org/10.1115/1.3250449.

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An experimental and theoretical study of the structure and radiation properties of luminous, round, turbulent acetylene/air diffusion flames is described. Measurements were made of mean and fluctuating velocities, mean concentrations, laser extinction (514 and 632.8 nm), spectral radiation intensities (1200–5500 nm), and radiative heat fluxes. The measurements were used to evaluate structure predictions based on the laminar flamelet concept, and radiation predictions based on a narrow-band model both ignoring and considering turbulence/radiation interactions. State relationships needed for the

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18

Li, Genong, and Michael F. Modest. "Application of composition PDF methods in the investigation of turbulence–radiation interactions." Journal of Quantitative Spectroscopy and Radiative Transfer 73, no. 2-5 (2002): 461–72. http://dx.doi.org/10.1016/s0022-4073(01)00218-7.

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19

Deshmukh, K. V., D. C. Haworth, and M. F. Modest. "Direct numerical simulation of turbulence–radiation interactions in homogeneous nonpremixed combustion systems." Proceedings of the Combustion Institute 31, no. 1 (2007): 1641–48. http://dx.doi.org/10.1016/j.proci.2006.07.139.

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20

Gu, Yu, and K. N. Liou. "Interactions of Radiation, Microphysics, and Turbulence in the Evolution of Cirrus Clouds." Journal of the Atmospheric Sciences 57, no. 15 (2000): 2463–79. http://dx.doi.org/10.1175/1520-0469(2000)057<2463:iormat>2.0.co;2.

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21

Chan, S. H., X. C. Pan, and J. Zhang. "Two-dimensional nonstationary causal stochastic model for turbulence/radiation interactions in flames." Symposium (International) on Combustion 25, no. 1 (1994): 1115–23. http://dx.doi.org/10.1016/s0082-0784(06)80749-6.

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22

Twomey, S. "Comments on “Interactions among Turbulence, Radiation and Microphysics in Arctic Stratus Clouds”." Journal of the Atmospheric Sciences 43, no. 22 (1986): 2752. http://dx.doi.org/10.1175/1520-0469(1986)043<2752:coatra>2.0.co;2.

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23

DEKA, P. N., and A. BORGOHAIN. "On unstable electromagnetic radiation through nonlinear wave–particle interactions in presence of drift wave turbulence." Journal of Plasma Physics 78, no. 5 (2012): 515–24. http://dx.doi.org/10.1017/s0022377812000207.

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AbstractA study on the generation of unstable electromagnetic wave through nonlinear wave–particle interactions in an inhomogeneous plasma has been presented. Drift wave turbulence, which is one of the common features of inhomogeneous plasma, is found to be strongly in phase relation with thermal particles. The plasma particles, accelerated by drift wave turbulence field, may transfer their energy to electromagnetic O-mode through a modulated field. This process has been described by Vlasov Maxwell system of equations. From the nonlinear dispersion relation for O-mode the growth rate has been

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24

Dos Santos, E. D., M. M. Galarça, A. C. Mossi, A. P. Petry, and F. H. R. França. "A NUMERICAL STUDY OF THE INFLUENCE OF TEMPERATURE FLUCTUATIONS IN THE THERMAL RADIATION FIELD." Revista de Engenharia Térmica 8, no. 1 (2009): 51. http://dx.doi.org/10.5380/reterm.v8i1.61882.

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The present paper performs a numerical study of the influence of fluctuations on the temperature field over the thermal radiation field with the purpose to simulate the effect of Turbulence-Radiation Interactions (TRI). To evaluate the behavior of the divergence of the radiant heat flux for a flame in a cylindrical cavity, four temperature profiles are imposed: an average temperature profile and other three with 10%, 20% and 30% of turbulence intensity. The radiative transfer equation is solved using the discrete ordinates method (DOM) and the participating medium is treated as a gray gas. The

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25

Gupta, A., D. C. Haworth, and M. F. Modest. "Turbulence-radiation interactions in large-eddy simulations of luminous and nonluminous nonpremixed flames." Proceedings of the Combustion Institute 34, no. 1 (2013): 1281–88. http://dx.doi.org/10.1016/j.proci.2012.05.052.

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26

Mazumder, Sandip, and Michael F. Modest. "A probability density function approach to modeling turbulence–radiation interactions in nonluminous flames." International Journal of Heat and Mass Transfer 42, no. 6 (1999): 971–91. http://dx.doi.org/10.1016/s0017-9310(98)00225-7.

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27

Krishnamoorthy, Gautham, and Md Ashiqur Rahman. "Assessing the role of turbulence-radiation interactions in hydrogen-enriched oxy-methane flames." International Journal of Hydrogen Energy 43, no. 11 (2018): 5722–36. http://dx.doi.org/10.1016/j.ijhydene.2018.01.157.

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28

Roger, Maxime, Carlos B. Da Silva, and Pedro J. Coelho. "Analysis of the turbulence–radiation interactions for large eddy simulations of turbulent flows." International Journal of Heat and Mass Transfer 52, no. 9-10 (2009): 2243–54. http://dx.doi.org/10.1016/j.ijheatmasstransfer.2008.12.004.

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29

Kitiashvili, Irina N. "Radiative hydrodynamic simulations of turbulent convection and pulsations of Kepler target stars." Proceedings of the International Astronomical Union 9, S301 (2013): 193–96. http://dx.doi.org/10.1017/s1743921313014312.

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AbstractThe problem of interaction of stellar pulsations with turbulence and radiation in stellar convective envelopes is central to our understanding of excitation mechanisms, oscillation amplitudes and frequency shifts. Realistic (“ab initio”) numerical simulations provide unique insights into the complex physics of pulsation-turbulence-radiation interactions, as well as into the energy transport and dynamics of convection zones, beyond the standard evolutionary theory. 3D radiative hydrodynamics simulations have been performed for several Kepler target stars, from M- to A-class along the ma

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30

Buchta, David A., Gregory Shallcross, and Jesse Capecelatro. "Sound and turbulence modulation by particles in high-speed shear flows." Journal of Fluid Mechanics 875 (July 18, 2019): 254–85. http://dx.doi.org/10.1017/jfm.2019.467.

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High-speed free-shear-flow turbulence, laden with droplets or particles, can radiate weaker pressure fluctuations than its unladen counterpart. In this study, Eulerian–Lagrangian simulations of high-speed temporally evolving shear layers laden with monodisperse, adiabatic, inertial particles are used to examine particle–turbulence interactions and their effect on radiated pressure fluctuations. An evolution equation for gas-phase pressure intensity is formulated for particle-laden flows, and local mechanisms of pressure changes are quantified over a range of Mach numbers and particle mass load

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31

Deshmukh, K. V., M. F. Modest, and D. C. Haworth. "Direct numerical simulation of turbulence–radiation interactions in a statistically one-dimensional nonpremixed system." Journal of Quantitative Spectroscopy and Radiative Transfer 109, no. 14 (2008): 2391–400. http://dx.doi.org/10.1016/j.jqsrt.2008.04.005.

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32

Miranda, Flavia C., Pedro J. Coelho, Francesca di Mare, and Johannes Janicka. "Study of turbulence-radiation interactions in large-eddy simulation of scaled Sandia flame D." Journal of Quantitative Spectroscopy and Radiative Transfer 228 (May 2019): 47–56. http://dx.doi.org/10.1016/j.jqsrt.2019.02.010.

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33

Zheng, Yuan, R. S. Barlow, and Jay P. Gore. "Measurements and Calculations of Spectral Radiation Intensities for Turbulent Non-Premixed and Partially Premixed Flames." Journal of Heat Transfer 125, no. 4 (2003): 678–86. http://dx.doi.org/10.1115/1.1589502.

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Spectral radiation intensities leaving diametric and chord-like paths for six non-sooting flames were measured using an infrared array spectrometer. The spectral radiation intensities were also computed using the mean property approach and a time and space series simulation approach. Turbulence/radiation interactions (TRI) in these flames were investigated by comparing the two sets of computations to the experimental data. The effects of TRI are significant for regions away from the flame axis. The new data and findings are of value in the evaluation of radiation models, which are increasingly

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34

Yang, Xiao, Zhihong He, Shikui Dong, and Heping Tan. "Prediction of turbulence radiation interactions of CH4H2/air turbulent flames at atmospheric and elevated pressures." International Journal of Hydrogen Energy 43, no. 32 (2018): 15537–50. http://dx.doi.org/10.1016/j.ijhydene.2018.06.060.

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35

Liu, L. H., X. Xu, and Y. L. Chen. "On the shapes of the presumed probability density function for the modeling of turbulence–radiation interactions." Journal of Quantitative Spectroscopy and Radiative Transfer 87, no. 3-4 (2004): 311–23. http://dx.doi.org/10.1016/j.jqsrt.2004.03.008.

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36

Mathew, Sajay Sunny, and Christoph Federrath. "The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation, and outflow feedback." Monthly Notices of the Royal Astronomical Society 507, no. 2 (2021): 2448–67. http://dx.doi.org/10.1093/mnras/stab2338.

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ABSTRACT We perform a series of three-dimensional, magnetohydrodynamical simulations of star cluster formation including gravity, turbulence, magnetic fields, stellar radiative heating, and outflow feedback. We observe that the inclusion of protostellar outflows (1) reduces the star formation rate by a factor of ∼2, (2) increases fragmentation, and (3) shifts the initial mass function (IMF) to lower masses by a factor of 2.0 ± 0.2, without significantly affecting the overall shape of the IMF. The form of the sink particle (protostellar objects) mass distribution obtained from our simulations m

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37

Wang, H., G. Y. Shi, X. Y. Zhang, et al. "Mesoscale modeling study of the interactions between aerosols and PBL meteorology during a haze episode in China Jing-Jin-Ji and its near surrounding region – Part 2: Aerosols' radiative feedback effects." Atmospheric Chemistry and Physics Discussions 14, no. 20 (2014): 28269–98. http://dx.doi.org/10.5194/acpd-14-28269-2014.

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Abstract. Two model experiments, namely a control (CTL) experiment without aerosol-radiation feedbacks and a RAD experiment with online aerosol-radiation interactions, were designed to study the radiative feedback on regional radiation budgets, PBL meteorology and haze formation due to aerosols during haze episodes over China Jing-Jin-Ji and its near surroundings (3JNS Region, for Beijing, Tianjin, Hebei Province, East Shanxi Province, West Shandong Province and North Henan Province) with a two-way atmospheric chemical transport model. The impact of aerosols on solar radiation reaching Earth's

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Wang, H., G. Y. Shi, X. Y. Zhang, et al. "Mesoscale modelling study of the interactions between aerosols and PBL meteorology during a haze episode in China Jing–Jin–Ji and its near surrounding region – Part 2: Aerosols' radiative feedback effects." Atmospheric Chemistry and Physics 15, no. 6 (2015): 3277–87. http://dx.doi.org/10.5194/acp-15-3277-2015.

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Abstract. Two model experiments, namely a control (CTL) experiment without aerosol–radiation feedbacks and a experiment with online aerosol–radiation (RAD) interactions, were designed to study the radiative feedback on regional radiation budgets, planetary boundary layer (PBL) meteorology and haze formation due to aerosols during haze episodes over Jing–Jin–Ji, China, and its near surroundings (3JNS region of China: Beijing, Tianjin, Hebei, East Shanxi, West Shandong and North Henan) with a two-way atmospheric chemical transport model. The impact of aerosols on solar radiation reaching Earth's

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39

Barcelos, Bernardo, and Felipe Centeno. "Numerical assessment of the effect of inflow turbulators on the thermal behavior of a combustion chamber." Thermal Science, no. 00 (2019): 323. http://dx.doi.org/10.2298/tsci181119323b.

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This work numerically investigates the effects of turbulators at the air and fuel (methane) inlets on the thermal behavior of a combustion chamber. Conservation equations for mass, momentum, energy, gaseous chemical species, soot, and temperature fluctuation variance in cylindrical axysimmetric coordinates were solved using the finite volume method. Chemical reaction rates were computed through the Arrhenius-Magnussen model, with two-step combustion reaction. The turbulence closure model, to compute the turbulent viscosity, was the standard ?-?. The modeling of turbulence-radiation interaction

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40

Song, Dehai, Wen Wu, and Qiang Li. "Effects of Wave–Current Interactions on Bay–Shelf Exchange." Journal of Physical Oceanography 51, no. 5 (2021): 1637–54. http://dx.doi.org/10.1175/jpo-d-20-0222.1.

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AbstractBay–shelf exchange is critical to coastal systems because it promotes self-purification or pollution dilution of the systems. In this study, the effects of wave–current interactions on bay–shelf exchange are explored in a micromesotidal system—Daya Bay in southern China. Waves can enlarge the shear-induced seaward transport and reduce the residual-current-induced landward transport, which benefits the bay–shelf exchange; however, tides work oppositely and slow the wave-induced bay–shelf exchange through vertical mixing and reduced shear-induced exchange. Five wave–current interactions

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41

Wood, Robert. "Stratocumulus Clouds." Monthly Weather Review 140, no. 8 (2012): 2373–423. http://dx.doi.org/10.1175/mwr-d-11-00121.1.

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Abstract This paper reviews the current knowledge of the climatological, structural, and organizational aspects of stratocumulus clouds and the physical processes controlling them. More of Earth’s surface is covered by stratocumulus clouds than by any other cloud type making them extremely important for Earth’s energy balance, primarily through their reflection of solar radiation. They are generally thin clouds, typically occupying the upper few hundred meters of the planetary boundary layer (PBL), and they preferably occur in shallow PBLs that are readily coupled by turbulent mixing to the su

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42

Roger, M., P. J. Coelho, and C. B. da Silva. "Relevance of the subgrid-scales for large eddy simulations of turbulence–radiation interactions in a turbulent plane jet." Journal of Quantitative Spectroscopy and Radiative Transfer 112, no. 7 (2011): 1250–56. http://dx.doi.org/10.1016/j.jqsrt.2010.08.026.

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43

Wang, Shouping, Qing Wang, Rachel E. Jordan, and P. O. G. Persson. "Interactions among longwave radiation of clouds, turbulence, and snow surface temperature in the Arctic: A model sensitivity study." Journal of Geophysical Research: Atmospheres 106, no. D14 (2001): 15323–33. http://dx.doi.org/10.1029/2000jd900358.

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Lohou, Fabienne, Norbert Kalthoff, Bianca Adler, et al. "Conceptual model of diurnal cycle of low-level stratiform clouds over southern West Africa." Atmospheric Chemistry and Physics 20, no. 4 (2020): 2263–75. http://dx.doi.org/10.5194/acp-20-2263-2020.

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Abstract. The DACCIWA (Dynamics Aerosol Chemistry Cloud Interactions in West Africa) project and the associated ground-based field experiment, which took place during summer 2016, provided a comprehensive dataset on the low-level stratiform clouds (LLSCs), which develop almost every night over southern West Africa. The LLSCs, inaccurately represented in climate and weather forecasts, form in the monsoon flow during the night and break up during the following morning or afternoon, affecting considerably the radiation budget. Several published studies give an overview of the measurements during

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45

Krafft, Catherine, Alexander S. Volokitin, and Gaëtan Gauthier. "Turbulence and Microprocesses in Inhomogeneous Solar Wind Plasmas." Fluids 4, no. 2 (2019): 69. http://dx.doi.org/10.3390/fluids4020069.

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The random density fluctuations observed in the solar wind plasma crucially influence on the Langmuir wave turbulence generated by energetic electron beams ejected during solar bursts. Those are powerful phenomena consisting of a chain of successive processes leading ultimately to strong electromagnetic emissions. The small-scale processes governing the interactions between the waves, the beams and the inhomogeneous plasmas need to be studied to explain such macroscopic phenomena. Moreover, the complexity induced by the plasma irregularities requires to find new approaches and modelling. There

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46

Zhdankin, Vladimir, Dmitri A. Uzdensky, Gregory R. Werner, and Mitchell C. Begelman. "Kinetic turbulence in shining pair plasma: intermittent beaming and thermalization by radiative cooling." Monthly Notices of the Royal Astronomical Society 493, no. 1 (2020): 603–26. http://dx.doi.org/10.1093/mnras/staa284.

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ABSTRACT High-energy astrophysical systems frequently contain collision-less relativistic plasmas that are heated by turbulent cascades and cooled by emission of radiation. Understanding the nature of this radiative turbulence is a frontier of extreme plasma astrophysics. In this paper, we use particle-in-cell simulations to study the effects of external inverse Compton radiation on turbulence driven in an optically thin, relativistic pair plasma. We focus on the statistical steady state (where injected energy is balanced by radiated energy) and perform a parameter scan spanning from low magne

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47

Schmidli, Juerg, Brian Billings, Fotini K. Chow, et al. "Intercomparison of Mesoscale Model Simulations of the Daytime Valley Wind System." Monthly Weather Review 139, no. 5 (2011): 1389–409. http://dx.doi.org/10.1175/2010mwr3523.1.

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Three-dimensional simulations of the daytime thermally induced valley wind system for an idealized valley–plain configuration, obtained from nine nonhydrostatic mesoscale models, are compared with special emphasis on the evolution of the along-valley wind. The models use the same initial and lateral boundary conditions, and standard parameterizations for turbulence, radiation, and land surface processes. The evolution of the mean along-valley wind (averaged over the valley cross section) is similar for all models, except for a time shift between individual models of up to 2 h and slight differ

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48

Werth, David, Robert Kurzeja, Nelson Luís Dias, et al. "The Simulation of the Southern Great Plains Nocturnal Boundary Layer and the Low-Level Jet with a High-Resolution Mesoscale Atmospheric Model." Journal of Applied Meteorology and Climatology 50, no. 7 (2011): 1497–513. http://dx.doi.org/10.1175/2011jamc2272.1.

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AbstractA field project over the Atmospheric Radiation Measurement–Cloud and Radiation Test Bed (ARM–CART) site during a period of several nights in September 2007 was conducted to explore the evolution of the low-level jet (LLJ). Data were collected from in situ (a multilevel tower) and remote (sodar) sensors, and the observed LLJ activity during the project was found to agree well with data from earlier studies regarding jet speed, height, and direction. To study nocturnal boundary layer (NBL) behavior, the Regional Atmospheric Modeling System was used to simulate the ARM–CART NBL field expe

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Gao, Guan Dong, Xiao Hua Wang, Dehai Song, et al. "Effects of Wave–Current Interactions on Suspended-Sediment Dynamics during Strong Wave Events in Jiaozhou Bay, Qingdao, China." Journal of Physical Oceanography 48, no. 5 (2018): 1053–78. http://dx.doi.org/10.1175/jpo-d-17-0259.1.

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AbstractWave–current interactions are crucial to suspended-sediment dynamics, but the roles of the associated physical mechanisms, the depth-dependent wave radiation stress, Stokes drift velocity, vertical transfer of wave-generated pressure transfer to the mean momentum equation (form drag), wave dissipation as a source term in the turbulence kinetic energy equation, and mean current advection and refraction of wave energy, have not yet been fully understood. Therefore, in this study, a computationally fast wave model developed by Mellor et al., a Finite Volume Coastal Ocean Model (FVCOM) hyd

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Goldstein, M. E., M. Z. Afsar, and S. J. Leib. "Non-homogeneous rapid distortion theory on transversely sheared mean flows." Journal of Fluid Mechanics 736 (November 8, 2013): 532–69. http://dx.doi.org/10.1017/jfm.2013.518.

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AbstractThis paper is concerned with the small-amplitude unsteady motion of an inviscid non-heat-conducting compressible fluid on a transversely sheared mean flow. It extends previous analyses (Goldstein,J. Fluid Mech., vol. 84, 1978b, pp. 305–329; Goldstein,J. Fluid Mech., vol. 91, 1979a, pp. 601–632), which show that the hydrodynamic component of the motion is determined by two arbitrary convected quantities in the absence of solid surfaces and hydrodynamic instabilities. These results can be used to specify appropriate upstream boundary conditions for unsteady surface interaction problems o

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