Planktonic microbes play a crucial role in the matter transformation and energy transfer of marine ecosystems.Marine microbial communities are profoundly influenced by various environmental factors,and their variation...Planktonic microbes play a crucial role in the matter transformation and energy transfer of marine ecosystems.Marine microbial communities are profoundly influenced by various environmental factors,and their variations are typically investigated in a time-dependent manner.However,studies conducted on a monthly or annual basis do not offer sufficient temporal resolution to reveal changes that can occur on an hourly basis.We conducted a high-resolution time-series study using amplicon sequencing on seawater samples taken at 2-h intervals over a 3-d period from the subtropical Daya Bay to investigate changes in the microbial community composition and activity.The results showed that 46.8%of the microbial rRNA sequences exhibited circadian rhythms,including phytoplankton(e.g.,Bacillariophyta,Cryptophyta,and Dinophyceae),heterotrophic bacteria(e.g.,Actinomarinaceae,Flavobacteriaceae,and SAR11_clade),and zooplankton(e.g.,Bestiolina and Phyllopharyngea).The genera of Bacillariophyta(e.g.,Chaetoceros and Pseudo-nitzschia)exhibited higher activity than those of Chlorophyta(e.g.,Micromonas).A similar trend was observed for zooplankton,where Choanozoa(e.g.,Copepoda)showed a strong circadian rhythm in abundance whereas Ciliophora(e.g.,Pithites)were more active.Light intensity and tides were identified as the driving factors behind the periodic succession and activity of the heterotrophic bacteria and phytoplankton with the exception of picocyanobacteria,which were mainly influenced by fluctuations in temperature,nutrients,and salinity.These high-resolution time-dependent observations showed that,despite the dynamic coastal environment,the periodic changes in the microbial community and activity were distinct and phylogenetically conserved.The findings may help in the development of ecosystem models for predicting microbial abundance and activity in rapidly changing coastal and estuary environments.展开更多
A memory reduction technique is proposed for solving stationary kinetic model equations. As implied by an integral solution of the stationary kinetic equation, a velocity distribution function can be reconstructed fro...A memory reduction technique is proposed for solving stationary kinetic model equations. As implied by an integral solution of the stationary kinetic equation, a velocity distribution function can be reconstructed from given macroscopic variables. Based on this fact, we propose a technique to reconstruct distribution function at discrete level, and employ it to develop an implicit numerical method for kinetic equations. The new implicit method only stores the macroscopic quantities which appear in the collision term, and does not store the distribution functions. As a result, enormous memory requirement for solving kinetic equations is totally relieved. Several boundary conditions, such as, inlet, outlet and isothermal boundaries, are discussed. Some numerical tests demonstrate the validity and efficiency of the technique.The new implicit solver provides nearly identical solution as the explicit kinetic solver, while the memory requirement is on the same order as the Navier–Stokes solver.展开更多
The Ellipsoidal Statistical model(ES-model)and the Shakhov model(S-model)were constructed to correct the Prandtl number of the original BGK model through the modification of stress and heatflux.With the introduction of ...The Ellipsoidal Statistical model(ES-model)and the Shakhov model(S-model)were constructed to correct the Prandtl number of the original BGK model through the modification of stress and heatflux.With the introduction of a new pa-rameter to combine the ES-model and S-model,a generalized kinetic model can be developed.This new model can give the correct Navier-Stokes equations in the con-tinuumflow regime.Through the adjustment of the new parameter,it provides abun-dant dynamic effect beyond the ES-model and S-model.Changing the free parameter,the physical performance of the new model has been tested numerically.The unified gas kinetic scheme(UGKS)is employed for the study of the new model.In transitionflow regime,many physical problems,i.e.,the shock structure and micro-flows,have been studied using the generalized model.With a careful choice of the free parameter,good results can be achieved for most test cases.Due to the property of the Boltz-mann collision integral,the new parameter in the generalized kinetic model cannot be fully determined.It depends on the specific problem.Generally speaking,the S-model predicts more accurate numerical solutions in most test cases presented in this paper than the ES-model,while ES-model performs better in the cases where theflow is mostly driven by temperature gradient,such as a channelflow with large boundary temperature variation at high Knudsen number.展开更多
In this paper,a well-balanced kinetic scheme for the gas dynamic equations under gravitational field is developed.In order to construct such a scheme,the physical process of particles transport through a potential bar...In this paper,a well-balanced kinetic scheme for the gas dynamic equations under gravitational field is developed.In order to construct such a scheme,the physical process of particles transport through a potential barrier at a cell interface is considered,where the amount of particle penetration and reflection is evaluated according to the incident particle velocity.This work extends the approach of Perthame and Simeoni for the shallow water equations[Calcolo,38(2001),pp.201-231]to the Euler equations under gravitational field.For an isolated system,this scheme is probably the only well-balanced method which can precisely preserve an isothermal steady state solution under time-independent gravitational potential.A few numerical examples are used to validate the above approach.展开更多
The paper introduces the gas-kinetic scheme for three-dimensional(3D)flow simulation.First,under a unified coordinate transformation,the 3D gaskinetic BGK equation is transformed into a computational space with arbitr...The paper introduces the gas-kinetic scheme for three-dimensional(3D)flow simulation.First,under a unified coordinate transformation,the 3D gaskinetic BGK equation is transformed into a computational space with arbitrary mesh moving velocity.Second,based on the Chapman-Enskog expansion of the kinetic equation,a local solution of gas distribution function is constructed and used in a finite volume scheme.As a result,a Navier-Stokes flow solver is developed for the low speed flow computation with dynamical mesh movement.Several test cases are used to validate the 3D gas-kinetic method.The first example is a 3D cavity flow with up-moving boundary at Reynolds number 3200,where the periodic solutions are compared with the experimental measurements.Then,the flow evolution inside a rotating 3D cavity is simulated with the moving mesh method,where the solution differences between 2D and 3D simulation are explicitly presented.Finally,the scheme is applied to the falling plate study,where the unsteady plate tumbling motion inside water tank has been studied and compared with the experimental measurements.展开更多
基金supported by the National Natural Science Foundation of China(grant nos.42141003,42276163,and 42321004)Shenzhen Science,Technology and Innovation Commission(SZSTI)Programme(grant nos.JCYJ20220530115401003,KCXFZ2021102017480305,and KCXFZ20211020174803005)+4 种基金Department of Science and Technology of Guangdong Province(grant no.2021B1515120080)Shenzhen Key Laboratory of Marine Archaea Geo-Omics,Southern University of Science and Technology(grant no.ZDSYS201802081843490)Project of Educational Commission of Guangdong Province of China(grant no.2020KTSCX123)Shanghai Sheshan National Geophysical Observatory(grant no.2020Z01)supported by Shanghai Frontiers Science Center of Polar Science(SCOPS,grant no.SOO2004-03).
文摘Planktonic microbes play a crucial role in the matter transformation and energy transfer of marine ecosystems.Marine microbial communities are profoundly influenced by various environmental factors,and their variations are typically investigated in a time-dependent manner.However,studies conducted on a monthly or annual basis do not offer sufficient temporal resolution to reveal changes that can occur on an hourly basis.We conducted a high-resolution time-series study using amplicon sequencing on seawater samples taken at 2-h intervals over a 3-d period from the subtropical Daya Bay to investigate changes in the microbial community composition and activity.The results showed that 46.8%of the microbial rRNA sequences exhibited circadian rhythms,including phytoplankton(e.g.,Bacillariophyta,Cryptophyta,and Dinophyceae),heterotrophic bacteria(e.g.,Actinomarinaceae,Flavobacteriaceae,and SAR11_clade),and zooplankton(e.g.,Bestiolina and Phyllopharyngea).The genera of Bacillariophyta(e.g.,Chaetoceros and Pseudo-nitzschia)exhibited higher activity than those of Chlorophyta(e.g.,Micromonas).A similar trend was observed for zooplankton,where Choanozoa(e.g.,Copepoda)showed a strong circadian rhythm in abundance whereas Ciliophora(e.g.,Pithites)were more active.Light intensity and tides were identified as the driving factors behind the periodic succession and activity of the heterotrophic bacteria and phytoplankton with the exception of picocyanobacteria,which were mainly influenced by fluctuations in temperature,nutrients,and salinity.These high-resolution time-dependent observations showed that,despite the dynamic coastal environment,the periodic changes in the microbial community and activity were distinct and phylogenetically conserved.The findings may help in the development of ecosystem models for predicting microbial abundance and activity in rapidly changing coastal and estuary environments.
基金supported by the National Natural Science Foundation of China(11602091 and 91530319)the National Key Research and Development Plan(2016YFB0600805)
文摘A memory reduction technique is proposed for solving stationary kinetic model equations. As implied by an integral solution of the stationary kinetic equation, a velocity distribution function can be reconstructed from given macroscopic variables. Based on this fact, we propose a technique to reconstruct distribution function at discrete level, and employ it to develop an implicit numerical method for kinetic equations. The new implicit method only stores the macroscopic quantities which appear in the collision term, and does not store the distribution functions. As a result, enormous memory requirement for solving kinetic equations is totally relieved. Several boundary conditions, such as, inlet, outlet and isothermal boundaries, are discussed. Some numerical tests demonstrate the validity and efficiency of the technique.The new implicit solver provides nearly identical solution as the explicit kinetic solver, while the memory requirement is on the same order as the Navier–Stokes solver.
基金This work was supported by Hong Kong Research Grant Council(621011,620813)SRFI11SC05 at HKUST and the National Natural Science Funds for Distin-guished Young Scholar group under Grant No.11221061.
文摘The Ellipsoidal Statistical model(ES-model)and the Shakhov model(S-model)were constructed to correct the Prandtl number of the original BGK model through the modification of stress and heatflux.With the introduction of a new pa-rameter to combine the ES-model and S-model,a generalized kinetic model can be developed.This new model can give the correct Navier-Stokes equations in the con-tinuumflow regime.Through the adjustment of the new parameter,it provides abun-dant dynamic effect beyond the ES-model and S-model.Changing the free parameter,the physical performance of the new model has been tested numerically.The unified gas kinetic scheme(UGKS)is employed for the study of the new model.In transitionflow regime,many physical problems,i.e.,the shock structure and micro-flows,have been studied using the generalized model.With a careful choice of the free parameter,good results can be achieved for most test cases.Due to the property of the Boltz-mann collision integral,the new parameter in the generalized kinetic model cannot be fully determined.It depends on the specific problem.Generally speaking,the S-model predicts more accurate numerical solutions in most test cases presented in this paper than the ES-model,while ES-model performs better in the cases where theflow is mostly driven by temperature gradient,such as a channelflow with large boundary temperature variation at high Knudsen number.
文摘In this paper,a well-balanced kinetic scheme for the gas dynamic equations under gravitational field is developed.In order to construct such a scheme,the physical process of particles transport through a potential barrier at a cell interface is considered,where the amount of particle penetration and reflection is evaluated according to the incident particle velocity.This work extends the approach of Perthame and Simeoni for the shallow water equations[Calcolo,38(2001),pp.201-231]to the Euler equations under gravitational field.For an isolated system,this scheme is probably the only well-balanced method which can precisely preserve an isothermal steady state solution under time-independent gravitational potential.A few numerical examples are used to validate the above approach.
基金supported by grants from the National Natural Science Foundation of China(Project No.10772033)K.Xu was supported by Hong Kong Research Grant Council 621709.
文摘The paper introduces the gas-kinetic scheme for three-dimensional(3D)flow simulation.First,under a unified coordinate transformation,the 3D gaskinetic BGK equation is transformed into a computational space with arbitrary mesh moving velocity.Second,based on the Chapman-Enskog expansion of the kinetic equation,a local solution of gas distribution function is constructed and used in a finite volume scheme.As a result,a Navier-Stokes flow solver is developed for the low speed flow computation with dynamical mesh movement.Several test cases are used to validate the 3D gas-kinetic method.The first example is a 3D cavity flow with up-moving boundary at Reynolds number 3200,where the periodic solutions are compared with the experimental measurements.Then,the flow evolution inside a rotating 3D cavity is simulated with the moving mesh method,where the solution differences between 2D and 3D simulation are explicitly presented.Finally,the scheme is applied to the falling plate study,where the unsteady plate tumbling motion inside water tank has been studied and compared with the experimental measurements.