The effect of the inlet gas pressure,supplementary gas pressure and nozzle channel dispersion angle on the pre-breakup behavior of Ti-6Al-4V(TC4)discontinuous droplets during EIGA was investigated by combining numeric...The effect of the inlet gas pressure,supplementary gas pressure and nozzle channel dispersion angle on the pre-breakup behavior of Ti-6Al-4V(TC4)discontinuous droplets during EIGA was investigated by combining numerical simulation with experiments.The results show that the axial velocity at the recirculation zone before the stagnation location was first increased and decreased then increased significantly after the peak value,while the pressure of the recirculation zone increased with the increase in inlet pressure.With the supplementary pressure increasing,the velocity magnitude and range of the recirculation zone gradually decreased.As the dispersion angle of the nozzle channel increased,the pre-breakup efficiency of droplets gradually decreased,but the adhesion phenomenon of droplets on the inner wall surface of the nozzle channel(IWSNC)gradually weakened.Under the inlet pressure of 4 MPa,a supplementary pressure of 0.05 MPa,and the dispersion angle of 15°,the uniform and spherical TC4 powders with diameter of 70μm were prepared,which was consistent with the simulation results.The optimized process parameters is a balance between the size of the pre-atomized particles and the back-spraying and bonding phenomenons of droplets.展开更多
塔北地区奥陶系碳酸盐岩缝洞型储层类型多样,探讨不同控制因素下的岩溶发育规律对岩溶缝洞油气勘探有重要意义。基于野外露头踏勘、岩心观察、薄片分析、岩溶充填物地球化学分析、测井成果分析,结合区域奥陶系走滑断裂解释、岩溶暴露期...塔北地区奥陶系碳酸盐岩缝洞型储层类型多样,探讨不同控制因素下的岩溶发育规律对岩溶缝洞油气勘探有重要意义。基于野外露头踏勘、岩心观察、薄片分析、岩溶充填物地球化学分析、测井成果分析,结合区域奥陶系走滑断裂解释、岩溶暴露期古地貌刻画、缝洞体静态刻画、生产动态数据成果分析,探讨岩溶类型较全的F I 7走滑断裂带的岩溶发育规律及其对储层和成藏的影响。结果表明:研究区岩溶流体主要为大气淡水,岩溶体系主要形成于加里东中晚期—海西早期,奥陶系一间房组、良里塔格组、桑塔木组暴露期形成大量古水系是岩溶发育的条件和岩溶作用结果;古地貌和走滑断裂在岩溶发育过程中起重要作用,古水系、地层尖灭线、地层碳酸盐岩含量、断裂发育程度等共同控制岩溶发育程度和分区特征;断裂带岩溶发育由北向南可依次划分为潜山岩溶区、顺层岩溶区、台缘叠加区、台缘陡坡排泄区、近岸斜坡断控区和远岸斜坡断控区;不同区带岩溶模式差异导致油气藏特点存在差异,通源断裂与优质缝洞储层匹配是区域油气成藏的关键因素。展开更多
The images captured by different observation station have different resolutions.The Helioseismic and Magnetic Imager(HMI:a part of the NASA Solar Dynamics Observatory SDO)has low-precision but wide coverage.And the Go...The images captured by different observation station have different resolutions.The Helioseismic and Magnetic Imager(HMI:a part of the NASA Solar Dynamics Observatory SDO)has low-precision but wide coverage.And the Goode Solar Telescope(GST,formerly known as the New Solar Telescope)at Big Bear Solar Observatory(BBSO)solar images has high precision but small coverage.The super-resolution can make the captured images become clearer,so it is wildly used in solar image processing.The traditional super-resolution methods,such as interpolation,often use single image’s feature to improve the image’s quality.The methods based on deep learning-based super-resolution image reconstruction algorithms have better quality,but small-scale features often become ambiguous.To solve this problem,a transitional amplification network structure is proposed.The network can use the two types images relationship to make the images clear.By adding a transition image with almost no difference between the source image and the target image,the transitional amplification training procedure includes three parts:transition image acquisition,transition network training with source images and transition images,and amplification network training with transition images and target images.In addition,the traditional evaluation indicators based on structural similarity(SSIM)and peak signal-to-noise ratio(PSNR)calculate the difference in pixel values and perform poorly in cross-type image reconstruction.The method based on feature matching can effectively evaluate the similarity and clarity of features.The experimental results show that the quality index of the reconstructed image is consistent with the visual effect.展开更多
基金Funded by the National Natural Science Foundation of China(No.51627805)the Natural Scienceof Guangdong Province,China(No.2015A030312003)the Science and Technology Research Project of Guangdong Province,China(No.2014B010129003)。
文摘The effect of the inlet gas pressure,supplementary gas pressure and nozzle channel dispersion angle on the pre-breakup behavior of Ti-6Al-4V(TC4)discontinuous droplets during EIGA was investigated by combining numerical simulation with experiments.The results show that the axial velocity at the recirculation zone before the stagnation location was first increased and decreased then increased significantly after the peak value,while the pressure of the recirculation zone increased with the increase in inlet pressure.With the supplementary pressure increasing,the velocity magnitude and range of the recirculation zone gradually decreased.As the dispersion angle of the nozzle channel increased,the pre-breakup efficiency of droplets gradually decreased,but the adhesion phenomenon of droplets on the inner wall surface of the nozzle channel(IWSNC)gradually weakened.Under the inlet pressure of 4 MPa,a supplementary pressure of 0.05 MPa,and the dispersion angle of 15°,the uniform and spherical TC4 powders with diameter of 70μm were prepared,which was consistent with the simulation results.The optimized process parameters is a balance between the size of the pre-atomized particles and the back-spraying and bonding phenomenons of droplets.
文摘塔北地区奥陶系碳酸盐岩缝洞型储层类型多样,探讨不同控制因素下的岩溶发育规律对岩溶缝洞油气勘探有重要意义。基于野外露头踏勘、岩心观察、薄片分析、岩溶充填物地球化学分析、测井成果分析,结合区域奥陶系走滑断裂解释、岩溶暴露期古地貌刻画、缝洞体静态刻画、生产动态数据成果分析,探讨岩溶类型较全的F I 7走滑断裂带的岩溶发育规律及其对储层和成藏的影响。结果表明:研究区岩溶流体主要为大气淡水,岩溶体系主要形成于加里东中晚期—海西早期,奥陶系一间房组、良里塔格组、桑塔木组暴露期形成大量古水系是岩溶发育的条件和岩溶作用结果;古地貌和走滑断裂在岩溶发育过程中起重要作用,古水系、地层尖灭线、地层碳酸盐岩含量、断裂发育程度等共同控制岩溶发育程度和分区特征;断裂带岩溶发育由北向南可依次划分为潜山岩溶区、顺层岩溶区、台缘叠加区、台缘陡坡排泄区、近岸斜坡断控区和远岸斜坡断控区;不同区带岩溶模式差异导致油气藏特点存在差异,通源断裂与优质缝洞储层匹配是区域油气成藏的关键因素。
基金This work was supported in part by CAS Key Laboratory of Solar Activity,National Astronomical Observatories Commission for Collaborating Research Program(CRP)(No:KLSA202114)National Science Foundation Project of P.R.China under Grant No.61701554+2 种基金the cross-discipline research project of Minzu University of China(2020MDJC08)State Language Commission Key Project(ZDl135-39)Promotion plan for young teachers scientific research ability of Minzu University of China,MUC 111 Project,First class courses(Digital Image Processing KC2066).
文摘The images captured by different observation station have different resolutions.The Helioseismic and Magnetic Imager(HMI:a part of the NASA Solar Dynamics Observatory SDO)has low-precision but wide coverage.And the Goode Solar Telescope(GST,formerly known as the New Solar Telescope)at Big Bear Solar Observatory(BBSO)solar images has high precision but small coverage.The super-resolution can make the captured images become clearer,so it is wildly used in solar image processing.The traditional super-resolution methods,such as interpolation,often use single image’s feature to improve the image’s quality.The methods based on deep learning-based super-resolution image reconstruction algorithms have better quality,but small-scale features often become ambiguous.To solve this problem,a transitional amplification network structure is proposed.The network can use the two types images relationship to make the images clear.By adding a transition image with almost no difference between the source image and the target image,the transitional amplification training procedure includes three parts:transition image acquisition,transition network training with source images and transition images,and amplification network training with transition images and target images.In addition,the traditional evaluation indicators based on structural similarity(SSIM)and peak signal-to-noise ratio(PSNR)calculate the difference in pixel values and perform poorly in cross-type image reconstruction.The method based on feature matching can effectively evaluate the similarity and clarity of features.The experimental results show that the quality index of the reconstructed image is consistent with the visual effect.
