The meteor radar can detect the zenith angle,azimuth,radial velocity,and altitude of meteor trails so that one can invert the wind profiles in the mesosphere and low thermosphere(MLT)region,based on the Interferometri...The meteor radar can detect the zenith angle,azimuth,radial velocity,and altitude of meteor trails so that one can invert the wind profiles in the mesosphere and low thermosphere(MLT)region,based on the Interferometric and Doppler techniques.In this paper,the horizontal wind field,gravity wave(GW)disturbance variance,and GW fluxes are analyzed through the meteor radar observation from 2012−2022,at Mohe(53.5°N,122.4°E)and Zuoling(30.5°N,114.6°E)stations of the(Chinese)Meridian Project.The Lomb−Scargle periodogram method has been utilized to analyze the periodic variations for time series with observational data gaps.The results show that the zonal winds at both stations are eastward dominated,while the meridional winds are southward dominated.The variance of GW disturbances in the zonal and meridional directions increases gradually with height,and there is a strong pattern of annual variation.The zonal momentum flux of GW changes little with height,showing weak annual variation.The meridional GW flux varies gradually from northward to southward with height,and the annual periodicity is stronger.For both stations,the maximum values of zonal and meridional wind occur close to the peak heights of GW flux,with opposite directions.This observational evidence is consistent with the filtering theory.The horizontal wind velocity,GW flux,and disturbance variance of the GW at Mohe are overall smaller than those at Zuoling,indicating weaker activities in the MLT at Mohe.The power spectral density(PSD)calculated by the Lomb−Scargle periodogram shows that there are 12-month period and 6-month period in horizontal wind field,GW disturbance variance and GW flux at both stations,and especially there is also a 4-month cycle in the disturbance variance.The PSD of the 12-month and 6-month cycles exhibits maximum values below 88 km and above 94 km.展开更多
We have developed a class of charged,anisotropic,and spherically symmetric solutions,described by the function f(R,A)=R+a A,where R represents the Ricci scalar,A is the anticurvature scalar,andαis the coupling consta...We have developed a class of charged,anisotropic,and spherically symmetric solutions,described by the function f(R,A)=R+a A,where R represents the Ricci scalar,A is the anticurvature scalar,andαis the coupling constant.The model was constructed using the Karmarkar condition to obtain the radial metric component,while the time metric component followed the approach proposed by Adler.We assumed a specific charge distribution inside the star to build the model.To ensure a smooth spacetime transition,we established boundary conditions,considering Bardeen?s solution for the exterior spacetime.Additionally,we examined various physical aspects,such as energy density,pressure components,pressure anisotropy,energy conditions,the equation of state,surface redshift,compactness factor,adiabatic index,sound speed,and the Tolman-Oppenheimer-Volkoff equilibrium condition.All these conditions were met,demonstrating that the solutions we obtained are physically viable.展开更多
In this article,a well-known anisotropic solution,the Tolman-Finch-Skea(TFS)solution,is studied using the gravitational decoupling approach within the framework of 4D Einstein-Gauss-Bonnet(EGB)gravity.The radial metri...In this article,a well-known anisotropic solution,the Tolman-Finch-Skea(TFS)solution,is studied using the gravitational decoupling approach within the framework of 4D Einstein-Gauss-Bonnet(EGB)gravity.The radial metric potential is modified linearly through the minimal geometric deformation approach,while the temporal component of the metric remains unchanged.The system of EGB field equations is decomposed into two distinct sets of field equations:one corresponding to the standard energy-momentum tensor and the other associated with an external gravitational source.The first system is solved using the aforementioned known solution,while the second is closed by imposing the mimic constraint on pressure.Moreover,the junction conditions at the inner and outer surfaces of the stellar object are examined,considering the Boulware-Deser 4D space-time as the external geometry.The physical properties of the stellar model are analyzed using parameters such as energy conditions,causality conditions,compactness,and redshift.展开更多
This study investigates the key characteristics of compact star configurations within the framework of Rastall’s theory of gravity,employing the Krori-Barua ansatz.By forming the field equations for a spherically sym...This study investigates the key characteristics of compact star configurations within the framework of Rastall’s theory of gravity,employing the Krori-Barua ansatz.By forming the field equations for a spherically symmetric line element with an isotropic matter source through Krori-Barua metric potentials,we derive the modified Tolman-Oppenheimer-Volkov equation.This equation is crucial for studying the mass-radius function,the compactness factor,and the surface redshift.Additionally,we examine various physical aspects,including energy density,pressure evolution,equation of state,adiabatic index,and stability analysis,to assess the model’s viability.Rastall’s theory,which extends general relativity by relaxing the conservation of energy and momentum,plays a central role in our analysis,particularly in understanding the enhanced stability of compact stars.Our results provide strong evidence that within Rastall’s gravitational framework,the proposed stellar structures exhibit significant stability,suggesting that this theory may offer new perspectives on the behavior of such stars.展开更多
Previous studies have indicated that sediment gravity flow deposits developed in lacustrine active extensional rift basins are primarily influenced by tectonics and to a lesser extent by climate.Our present work revea...Previous studies have indicated that sediment gravity flow deposits developed in lacustrine active extensional rift basins are primarily influenced by tectonics and to a lesser extent by climate.Our present work reveals that climate can obscure the effect of tectonic subsidence by regulating sediment supply;conversely,tectonics can impede the sedimentary manifestation of climatic impacts.Here a case study has been presented to assess the impact of climate-modulated rapid lake-level rise and tectonic subsidence on the development of coarse-grained gravity flow deposits in the Dongying rift margin of the Bohai Bay Basin,eastern China.The lithofacies analysis reveals frequent bed amalgamation,abundant thick massive coarse-grained deposits,widespread cross bedding and plant fragments,and incomplete composite bed formed by high-energy erosion,indicating that the hyperpycnal flow is an important mechanism driving the deposition of these coarse-grained sediments.Detailed sequence stratigraphic analysis and sediment dispersal pattern suggest that the long-striped nearshore subaqueous fan systems induced by outburst-flood hyperpycnal flow distributed along the border fault,are primarily controlled by long-term tectonics,while the rapid rise of lake level driven by short-term climate change possibly intensifies seasonal flood-generated hyperpycnal flow occurrences and consequently promotes the basinal fan progradation.The maximum scale of these coarse-grained gravity flow deposits of the basinal fan systems are typically attained during the transgressive systems tract,which deviates from the classical sequence stratigraphic model.Furthermore,it presented a continuous transition from the proximal to the distal part,encompassing traction flows and turbidity currents during the periods of relatively stable tectonics.Nevertheless,gravel-rich debris flows appear to predominate the dispersion of coarse-grained sediments during periods characterized by intense tectonic activity.The coarse-grained gravity flow deposits in the lacustrine rift margin reported here,challenge the traditional beliefs:this study suggests that subaqueous deposits abundantly preserved in the transgressive setting.展开更多
Based on the Many Worlds Interpretation,I describe reality as a multilayer spacetime,where parallel layers play the role of alternative timelines.I link physics to ethics,arguing that one’s moral choices shape one’s...Based on the Many Worlds Interpretation,I describe reality as a multilayer spacetime,where parallel layers play the role of alternative timelines.I link physics to ethics,arguing that one’s moral choices shape one’s course in the multiverse.I consider one’s ethical decisions as decoherence events,leading to movement between alternative timelines,lighter(higher)or heavier(lower)realities.Sometimes in one’s curvilinear path in spacetime,one can even experience falling toward lower layers,slipping through wormholes.This theory supports free will and the simulation hypothesis.With this background,I explore the idea that a new theory of gravity might open new possibilities to shape matter and change our worldview through the invention of new technology,transforming information into waves and then into solid matter,paving the way for a new Multiverse Aeon for humanity.展开更多
Tight glutenite reservoirs are known for strong heterogeneity,complex wettability,and challenging development.Gas-Assisted Gravity Drainage(GAGD)technology has the potential to significantly improve recovery efficienc...Tight glutenite reservoirs are known for strong heterogeneity,complex wettability,and challenging development.Gas-Assisted Gravity Drainage(GAGD)technology has the potential to significantly improve recovery efficiency in glutenite reservoir.However,there is currently limited research on GAGD processes specifically designed for glutenite reservoirs,and there is a lack of relevant dimensionless numbers for predicting recovery efficiency.In this study,we developed a theoretical model based on the characteristics of glutenite reservoirs and used phase-field method to track the oil-gas interface for numerical simulations of dynamic GAGD processes.To explore the factors influencing gas-driven recovery,we simulated the effects of strong heterogeneity and dynamic wettability on the construction process under gravity assistance.Additionally,we introduced multiple dimensionless numbers(including capillary number,viscosity ratio,and Bond number)and conducted a series of numerical simulations.The results demonstrate that gravity enhances the stability of the oil-gas interface but causes unstable pressure fluctuations when passing through different-sized throat regions,particularly leading to front advancement in smaller throats.Although strong heterogeneity has negative impacts on GAGD,they can be mitigated by reducing injection velocity.Increasing oil-wettability promotes oil displacement by overcoming capillary forces,particularly in narrower pores,allowing residual oils to be expelled.Among the dimensionless numbers,the recovery efficiency is directly proportional to the Bond number and inversely proportional to the capillary number and viscosity ratio.Through sensitivity analysis of the dimensionless numbers’impact on the recovery efficiency,a new dimensionless N_(Glu) considering heterogeneity is proposed to accurately predict GAGD recovery of tight glutenite reservoirs.展开更多
Using a recognition model of atmospheric gravity waves(AGWs),we identified 519 AGW events from the OH airglow images observed at the Dandong and Lhasa stations from 2015 to 2017.The 317 AGW events detected at the Dand...Using a recognition model of atmospheric gravity waves(AGWs),we identified 519 AGW events from the OH airglow images observed at the Dandong and Lhasa stations from 2015 to 2017.The 317 AGW events detected at the Dandong station have wavelengths ranging from 30 to 60 km,periods from 14 to 20 min,horizontal speeds from 30 to 60 m/s,and relative intensities from 0.4%to 0.6%,respectively.The parameters of 202 events recorded at the Lhasa station mainly vary within 15-35 km in horizontal wavelength,4-6 min in period,40-100 m/s in horizontal velocity,and 0.1%-0.3%in relative intensity.The occurrence rate peaks in winter and summer at Dandong and the peak in summer are absent at Lhasa because of the lack of convective weather.The seasonal propagation directions of the waves are influenced by both the wind field-filtering effect and the distribution of wave sources.In spring,because of the southeastward background wind field,fewer southeastward events are observed at the Dandong station.The situation at the Lhasa station is similar.In summer,both the Lhasa and Dandong stations are dominated by northeastward AGWs,which can be attributed to the southwestward wind.In autumn,ray-tracing results show that the events at Dandong mainly originate from wind shear,whereas the events at the Lhasa station are triggered by convective weather.The location of the wave sources determines the trend of the propagation directions at the Dandong and Lhasa stations in autumn.In winter,because of the eastward wind,more events are propagating to the southwest at the Dandong station.展开更多
The melting process of a phase change material(PCM) inside a capsule can be promising in the thermal management of spacecraft. Such spacecraft operate under various gravity conditions, but previous studies have mostly...The melting process of a phase change material(PCM) inside a capsule can be promising in the thermal management of spacecraft. Such spacecraft operate under various gravity conditions, but previous studies have mostly considered the influence of gravity conditions on the constrained melting process of a PCM and not on its unconstrained melting process. In this study, a numerical model was constructed to comprehensively analyze the constrained and unconstrained melting processes of a PCM inside a spherical capsule under low-gravity conditions. After validation, the model was then applied to investigating the effects of low-gravity conditions on the evolution of velocity, temperature, melt layer thickness, heat transfer, liquid fraction, and total melting time. For the unconstrained melting process, low-gravity conditions weaken buoyancy-driven natural convection and slow down the solid PCM downward trend, thereby limiting the melting rate. In addition, the melt layer thickness does not increase linearly with decreasing gravity. Specifically, the increase in melt layer thickness is smaller by about 1.06 mm when the gravity drops from 0.4g to 0.2g compared to when it drops from 0.2g to 0.1g. The local heat flux in the contact melting area gradually decreases with the reduction of gravity during the unconstrained melting process. During the constrained melting process, notable oscillations in the local heat flux were observed. Decreasing the gravity from g to 0g increased the total melting times of the constrained and unconstrained melting processes by 417% and 621%, respectively.展开更多
BACKGROUND Crohn’s disease(CD)is a chronic inflammatory bowel disease with unknown etiology.Inflammatory chemical mediators synthesized from arachidonic acid,an n-6 polyunsaturated fatty acid(PUFA),have been shown to...BACKGROUND Crohn’s disease(CD)is a chronic inflammatory bowel disease with unknown etiology.Inflammatory chemical mediators synthesized from arachidonic acid,an n-6 polyunsaturated fatty acid(PUFA),have been shown to activate CD.Additionally,n-3 PUFAs are metabolized by the same enzyme as n-6 PUFAs and known to inhibit the arachidonic acid cascade.Our previous study noted that the presence of erythrocyte membrane fatty acids is a characteristic finding in Japanese CD patients.It was thus speculated that FADS2 gene polymorphisms,which induce PUFA metabolizing enzymes,are involved in the pathogenesis of CD,though no such relationship was found.AIM To investigate the relationship of FADS2 polymorphisms with serum and erythrocyte membrane fatty acid composition ratios,and disease activity.METHODS Using previously reported findings regarding FADS2 genetic polymorphisms,the records of 52 CD patients undergoing treatment at Jikei University Kashiwa Hospital were analyzed.Mutations noted were divided into three groups;wild-type(GG),heterozygous mutants(GA),and homozygous(AA),with the activities of delta-6 and delta-5 desaturases compared using redefined d6d index(rd.d6di)and d5d index(d5di).Additionally,comparisons of serum and erythrocyte membranes for fatty acid composition,and also gene polymorphisms and CD activity index(CDAI)were performed.RESULTS The presence of the rs174538 mutation in FADS2 resulted in reduction of only rd.d6di in the erythrocyte membrane(P<0.01).In contrast,that mutation was found to be associated with d5di induced by FADS1 in serum(P=0.019)as well as the erythrocyte membrane(P<0.0001),and also with reduction in the fatty acid composition of arachidonic acid in both serum(P<0.0001)and the erythrocyte membrane(P<0.01).Regarding disease activity,a positive correlation of CDAI score with rd.d6di in both serum(P<0.05)and the erythrocyte membrane(P<0.05)was found only in the rs174538 wild-type group.In contrast,there was no correction between CDAI and d5di in either serum or erythrocyte membrane samples.CONCLUSION The rs174538 mutation alters the fatty acid profile through strong linkage to the FADS1 gene.In wild-type individuals,rd.d6di was positively correlated with CDAI,suggesting predictive utility of disease severity.展开更多
We present a method to calculate the full gravity gradient tensors from pre-existing vertical gravity data using the cosine transform technique and discuss the calculated tensor accuracy when the gravity anomalies are...We present a method to calculate the full gravity gradient tensors from pre-existing vertical gravity data using the cosine transform technique and discuss the calculated tensor accuracy when the gravity anomalies are contaminated by noise. Gravity gradient tensors computation on 2D infinite horizontal cylinder and 3D ＂Y＂ type dyke models show that the results computed with the DCT technique are more accurate than the FFT technique regardless if the gravity anomalies are contaminated by noise or not. The DCT precision has increased 2 to 3 times from the standard deviation. In application, the gravity gradient tensors of the Hulin basin calculated by DCT and FFT show that the two results are consistent with each other. However, the DCT results are smoother than results computed with FFT. This shows that the proposed method is less affected by noise and can better reflect the fault distribution.展开更多
基金supported by the Fundamental Research Funds for the Central Universities,CHD(NO.300102263205 and NO.300102264916)the West Light Cross-Disciplinary Innovation team of Chinese Academy of Sciences(NO.E1294301).supported by the Fundamental Research Funds for the Central Universities,CHD(NO.300102263205 and NO.300102264916)the West Light Cross-Disciplinary Innovation team of Chinese Academy of Sciences(NO.E1294301).
文摘The meteor radar can detect the zenith angle,azimuth,radial velocity,and altitude of meteor trails so that one can invert the wind profiles in the mesosphere and low thermosphere(MLT)region,based on the Interferometric and Doppler techniques.In this paper,the horizontal wind field,gravity wave(GW)disturbance variance,and GW fluxes are analyzed through the meteor radar observation from 2012−2022,at Mohe(53.5°N,122.4°E)and Zuoling(30.5°N,114.6°E)stations of the(Chinese)Meridian Project.The Lomb−Scargle periodogram method has been utilized to analyze the periodic variations for time series with observational data gaps.The results show that the zonal winds at both stations are eastward dominated,while the meridional winds are southward dominated.The variance of GW disturbances in the zonal and meridional directions increases gradually with height,and there is a strong pattern of annual variation.The zonal momentum flux of GW changes little with height,showing weak annual variation.The meridional GW flux varies gradually from northward to southward with height,and the annual periodicity is stronger.For both stations,the maximum values of zonal and meridional wind occur close to the peak heights of GW flux,with opposite directions.This observational evidence is consistent with the filtering theory.The horizontal wind velocity,GW flux,and disturbance variance of the GW at Mohe are overall smaller than those at Zuoling,indicating weaker activities in the MLT at Mohe.The power spectral density(PSD)calculated by the Lomb−Scargle periodogram shows that there are 12-month period and 6-month period in horizontal wind field,GW disturbance variance and GW flux at both stations,and especially there is also a 4-month cycle in the disturbance variance.The PSD of the 12-month and 6-month cycles exhibits maximum values below 88 km and above 94 km.
基金Deanship of Research and Graduate Studies at King Khalid University for funding this work through Large Research Project under Grant No.RGP2/30/45。
文摘We have developed a class of charged,anisotropic,and spherically symmetric solutions,described by the function f(R,A)=R+a A,where R represents the Ricci scalar,A is the anticurvature scalar,andαis the coupling constant.The model was constructed using the Karmarkar condition to obtain the radial metric component,while the time metric component followed the approach proposed by Adler.We assumed a specific charge distribution inside the star to build the model.To ensure a smooth spacetime transition,we established boundary conditions,considering Bardeen?s solution for the exterior spacetime.Additionally,we examined various physical aspects,such as energy density,pressure components,pressure anisotropy,energy conditions,the equation of state,surface redshift,compactness factor,adiabatic index,sound speed,and the Tolman-Oppenheimer-Volkoff equilibrium condition.All these conditions were met,demonstrating that the solutions we obtained are physically viable.
基金partially supported by the National Natural Science Foundation of China under Grant No.11988101。
文摘In this article,a well-known anisotropic solution,the Tolman-Finch-Skea(TFS)solution,is studied using the gravitational decoupling approach within the framework of 4D Einstein-Gauss-Bonnet(EGB)gravity.The radial metric potential is modified linearly through the minimal geometric deformation approach,while the temporal component of the metric remains unchanged.The system of EGB field equations is decomposed into two distinct sets of field equations:one corresponding to the standard energy-momentum tensor and the other associated with an external gravitational source.The first system is solved using the aforementioned known solution,while the second is closed by imposing the mimic constraint on pressure.Moreover,the junction conditions at the inner and outer surfaces of the stellar object are examined,considering the Boulware-Deser 4D space-time as the external geometry.The physical properties of the stellar model are analyzed using parameters such as energy conditions,causality conditions,compactness,and redshift.
基金The author,FM,expresses her gratitude to Princess Nourah bint Abdulrahman University Researchers Supporting Project No.(PNURSP2025R27),Princess Nourah bint Abdulrahman University,Riyadh,Saudi Arabia.
文摘This study investigates the key characteristics of compact star configurations within the framework of Rastall’s theory of gravity,employing the Krori-Barua ansatz.By forming the field equations for a spherically symmetric line element with an isotropic matter source through Krori-Barua metric potentials,we derive the modified Tolman-Oppenheimer-Volkov equation.This equation is crucial for studying the mass-radius function,the compactness factor,and the surface redshift.Additionally,we examine various physical aspects,including energy density,pressure evolution,equation of state,adiabatic index,and stability analysis,to assess the model’s viability.Rastall’s theory,which extends general relativity by relaxing the conservation of energy and momentum,plays a central role in our analysis,particularly in understanding the enhanced stability of compact stars.Our results provide strong evidence that within Rastall’s gravitational framework,the proposed stellar structures exhibit significant stability,suggesting that this theory may offer new perspectives on the behavior of such stars.
基金supported by the National Natural Science Foundation of China(Nos.42172109,41872113,42172108)China National Petroleum Corporation-China University of Petroleum(Beijing)strategic cooperation science and technology project(ZLZX2020-02)+2 种基金Science Foundation of China University of Petroleum(Beijing)(Nos.2462020BJRC002,2462020YXZZ020)Natural Science Foundation of Chongqing(CSTB2022NSCQ-MSX1166)Science and Technology Research Program of Chongqing Municipal Education Commission(KJQN202201511).
文摘Previous studies have indicated that sediment gravity flow deposits developed in lacustrine active extensional rift basins are primarily influenced by tectonics and to a lesser extent by climate.Our present work reveals that climate can obscure the effect of tectonic subsidence by regulating sediment supply;conversely,tectonics can impede the sedimentary manifestation of climatic impacts.Here a case study has been presented to assess the impact of climate-modulated rapid lake-level rise and tectonic subsidence on the development of coarse-grained gravity flow deposits in the Dongying rift margin of the Bohai Bay Basin,eastern China.The lithofacies analysis reveals frequent bed amalgamation,abundant thick massive coarse-grained deposits,widespread cross bedding and plant fragments,and incomplete composite bed formed by high-energy erosion,indicating that the hyperpycnal flow is an important mechanism driving the deposition of these coarse-grained sediments.Detailed sequence stratigraphic analysis and sediment dispersal pattern suggest that the long-striped nearshore subaqueous fan systems induced by outburst-flood hyperpycnal flow distributed along the border fault,are primarily controlled by long-term tectonics,while the rapid rise of lake level driven by short-term climate change possibly intensifies seasonal flood-generated hyperpycnal flow occurrences and consequently promotes the basinal fan progradation.The maximum scale of these coarse-grained gravity flow deposits of the basinal fan systems are typically attained during the transgressive systems tract,which deviates from the classical sequence stratigraphic model.Furthermore,it presented a continuous transition from the proximal to the distal part,encompassing traction flows and turbidity currents during the periods of relatively stable tectonics.Nevertheless,gravel-rich debris flows appear to predominate the dispersion of coarse-grained sediments during periods characterized by intense tectonic activity.The coarse-grained gravity flow deposits in the lacustrine rift margin reported here,challenge the traditional beliefs:this study suggests that subaqueous deposits abundantly preserved in the transgressive setting.
文摘Based on the Many Worlds Interpretation,I describe reality as a multilayer spacetime,where parallel layers play the role of alternative timelines.I link physics to ethics,arguing that one’s moral choices shape one’s course in the multiverse.I consider one’s ethical decisions as decoherence events,leading to movement between alternative timelines,lighter(higher)or heavier(lower)realities.Sometimes in one’s curvilinear path in spacetime,one can even experience falling toward lower layers,slipping through wormholes.This theory supports free will and the simulation hypothesis.With this background,I explore the idea that a new theory of gravity might open new possibilities to shape matter and change our worldview through the invention of new technology,transforming information into waves and then into solid matter,paving the way for a new Multiverse Aeon for humanity.
基金supported by the National Natural Science Foundation of China(U22B2075)the Fundamental Research Funds for the Central Universities(2024ZKPYSB03)support from Beijing University of Science and Technology.
文摘Tight glutenite reservoirs are known for strong heterogeneity,complex wettability,and challenging development.Gas-Assisted Gravity Drainage(GAGD)technology has the potential to significantly improve recovery efficiency in glutenite reservoir.However,there is currently limited research on GAGD processes specifically designed for glutenite reservoirs,and there is a lack of relevant dimensionless numbers for predicting recovery efficiency.In this study,we developed a theoretical model based on the characteristics of glutenite reservoirs and used phase-field method to track the oil-gas interface for numerical simulations of dynamic GAGD processes.To explore the factors influencing gas-driven recovery,we simulated the effects of strong heterogeneity and dynamic wettability on the construction process under gravity assistance.Additionally,we introduced multiple dimensionless numbers(including capillary number,viscosity ratio,and Bond number)and conducted a series of numerical simulations.The results demonstrate that gravity enhances the stability of the oil-gas interface but causes unstable pressure fluctuations when passing through different-sized throat regions,particularly leading to front advancement in smaller throats.Although strong heterogeneity has negative impacts on GAGD,they can be mitigated by reducing injection velocity.Increasing oil-wettability promotes oil displacement by overcoming capillary forces,particularly in narrower pores,allowing residual oils to be expelled.Among the dimensionless numbers,the recovery efficiency is directly proportional to the Bond number and inversely proportional to the capillary number and viscosity ratio.Through sensitivity analysis of the dimensionless numbers’impact on the recovery efficiency,a new dimensionless N_(Glu) considering heterogeneity is proposed to accurately predict GAGD recovery of tight glutenite reservoirs.
基金supported by the National Key Research and Development Program of China(Grant No.2022YFF0711402)the Specialized Research Fund for State Key Laboratories。
文摘Using a recognition model of atmospheric gravity waves(AGWs),we identified 519 AGW events from the OH airglow images observed at the Dandong and Lhasa stations from 2015 to 2017.The 317 AGW events detected at the Dandong station have wavelengths ranging from 30 to 60 km,periods from 14 to 20 min,horizontal speeds from 30 to 60 m/s,and relative intensities from 0.4%to 0.6%,respectively.The parameters of 202 events recorded at the Lhasa station mainly vary within 15-35 km in horizontal wavelength,4-6 min in period,40-100 m/s in horizontal velocity,and 0.1%-0.3%in relative intensity.The occurrence rate peaks in winter and summer at Dandong and the peak in summer are absent at Lhasa because of the lack of convective weather.The seasonal propagation directions of the waves are influenced by both the wind field-filtering effect and the distribution of wave sources.In spring,because of the southeastward background wind field,fewer southeastward events are observed at the Dandong station.The situation at the Lhasa station is similar.In summer,both the Lhasa and Dandong stations are dominated by northeastward AGWs,which can be attributed to the southwestward wind.In autumn,ray-tracing results show that the events at Dandong mainly originate from wind shear,whereas the events at the Lhasa station are triggered by convective weather.The location of the wave sources determines the trend of the propagation directions at the Dandong and Lhasa stations in autumn.In winter,because of the eastward wind,more events are propagating to the southwest at the Dandong station.
基金supported by the National Natural Science Foundation of China (Grant No.52376181)。
文摘The melting process of a phase change material(PCM) inside a capsule can be promising in the thermal management of spacecraft. Such spacecraft operate under various gravity conditions, but previous studies have mostly considered the influence of gravity conditions on the constrained melting process of a PCM and not on its unconstrained melting process. In this study, a numerical model was constructed to comprehensively analyze the constrained and unconstrained melting processes of a PCM inside a spherical capsule under low-gravity conditions. After validation, the model was then applied to investigating the effects of low-gravity conditions on the evolution of velocity, temperature, melt layer thickness, heat transfer, liquid fraction, and total melting time. For the unconstrained melting process, low-gravity conditions weaken buoyancy-driven natural convection and slow down the solid PCM downward trend, thereby limiting the melting rate. In addition, the melt layer thickness does not increase linearly with decreasing gravity. Specifically, the increase in melt layer thickness is smaller by about 1.06 mm when the gravity drops from 0.4g to 0.2g compared to when it drops from 0.2g to 0.1g. The local heat flux in the contact melting area gradually decreases with the reduction of gravity during the unconstrained melting process. During the constrained melting process, notable oscillations in the local heat flux were observed. Decreasing the gravity from g to 0g increased the total melting times of the constrained and unconstrained melting processes by 417% and 621%, respectively.
文摘BACKGROUND Crohn’s disease(CD)is a chronic inflammatory bowel disease with unknown etiology.Inflammatory chemical mediators synthesized from arachidonic acid,an n-6 polyunsaturated fatty acid(PUFA),have been shown to activate CD.Additionally,n-3 PUFAs are metabolized by the same enzyme as n-6 PUFAs and known to inhibit the arachidonic acid cascade.Our previous study noted that the presence of erythrocyte membrane fatty acids is a characteristic finding in Japanese CD patients.It was thus speculated that FADS2 gene polymorphisms,which induce PUFA metabolizing enzymes,are involved in the pathogenesis of CD,though no such relationship was found.AIM To investigate the relationship of FADS2 polymorphisms with serum and erythrocyte membrane fatty acid composition ratios,and disease activity.METHODS Using previously reported findings regarding FADS2 genetic polymorphisms,the records of 52 CD patients undergoing treatment at Jikei University Kashiwa Hospital were analyzed.Mutations noted were divided into three groups;wild-type(GG),heterozygous mutants(GA),and homozygous(AA),with the activities of delta-6 and delta-5 desaturases compared using redefined d6d index(rd.d6di)and d5d index(d5di).Additionally,comparisons of serum and erythrocyte membranes for fatty acid composition,and also gene polymorphisms and CD activity index(CDAI)were performed.RESULTS The presence of the rs174538 mutation in FADS2 resulted in reduction of only rd.d6di in the erythrocyte membrane(P<0.01).In contrast,that mutation was found to be associated with d5di induced by FADS1 in serum(P=0.019)as well as the erythrocyte membrane(P<0.0001),and also with reduction in the fatty acid composition of arachidonic acid in both serum(P<0.0001)and the erythrocyte membrane(P<0.01).Regarding disease activity,a positive correlation of CDAI score with rd.d6di in both serum(P<0.05)and the erythrocyte membrane(P<0.05)was found only in the rs174538 wild-type group.In contrast,there was no correction between CDAI and d5di in either serum or erythrocyte membrane samples.CONCLUSION The rs174538 mutation alters the fatty acid profile through strong linkage to the FADS1 gene.In wild-type individuals,rd.d6di was positively correlated with CDAI,suggesting predictive utility of disease severity.
基金supported by the Scientific Research Starting Foundation of HoHai University,China(2084/40801136)the Fundamental Research Funds for the Central Universities(No.2009B12514)
文摘We present a method to calculate the full gravity gradient tensors from pre-existing vertical gravity data using the cosine transform technique and discuss the calculated tensor accuracy when the gravity anomalies are contaminated by noise. Gravity gradient tensors computation on 2D infinite horizontal cylinder and 3D ＂Y＂ type dyke models show that the results computed with the DCT technique are more accurate than the FFT technique regardless if the gravity anomalies are contaminated by noise or not. The DCT precision has increased 2 to 3 times from the standard deviation. In application, the gravity gradient tensors of the Hulin basin calculated by DCT and FFT show that the two results are consistent with each other. However, the DCT results are smoother than results computed with FFT. This shows that the proposed method is less affected by noise and can better reflect the fault distribution.
