In order to study the effects of controlled release nitrogen fertilizer (CRNF) application on rapeseed, a simulated experiment was carried out with 3 types of paddy soils in Dongting Lake area for 4 consecutive year...In order to study the effects of controlled release nitrogen fertilizer (CRNF) application on rapeseed, a simulated experiment was carried out with 3 types of paddy soils in Dongting Lake area for 4 consecutive years of applying CRNF under double rice cropping system after planting rapeseed crop in the fallow season. The effects of CRNF application on rapeseed yield, agronomic characters and soil fertility were studied in this paper. The results showed that CRNF application improved the growth of rapeseed plant and increased rapeseed yield of CRNF treatments in the purple calcareous clayed paddy soil (PCS) and alluvial loamy paddy soil (ALS) which respectively increased by 12.2% and 9.8% compared with applying urea, re- spectively. The rapeseed yield in 70% CRNF treatment obviously decreased com- pared with urea treatment. The contents of available N and organic carbon in soil increased by 25.0% and 3.2% in CRNF treatment in the ALS after rapeseed crop, respectively; and available N increased by 13.5% in the PCS. Both rapeseed yield and soil fertility in CRNF treatment and 70% CRNF treatment were lower than those in CK treatment in the reddish yellow clayed paddy soil (RYS). The results al- so indicated that the functions of CRNF application on rapeseed yield increase and soil nitrogen fertility improvement were very obvious in the PCS and ALS.展开更多
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By analyzing Chandra X-ray data of a sample of 21 galaxy groups and 19 galaxy clusters, we find that in 31 sample systems there exists a significant central (R ≤ 10 h^-171 kpc) gas entropy excess (AK0), which cor...By analyzing Chandra X-ray data of a sample of 21 galaxy groups and 19 galaxy clusters, we find that in 31 sample systems there exists a significant central (R ≤ 10 h^-171 kpc) gas entropy excess (AK0), which corresponds to = 0.1 - 0.5 keV per gas particle, beyond the power-law model that best fits the radial entropy profile of the outer regions. We also find a distinct correlation between the central entropy excess △K0 and K-band luminosity LK of the central dominating galaxies (CDGs), which is scaled as △K0 ∝ L K 1.6±04, where LK is tightly associated with the mass of the supermassive black hole hosted in the CDG. In fact, if an effective mass-to-energy conversionefficiency of 0.02 is assumed for the accretion process, the cumulative AGN feedback E AGN feedack=ηMBHc2 yields an extra heating of = 0.5 - 17.0keV per particle, which feedback is sufficient to explain the central entropy excess. In most cases, the AGN contribution can compensate the radiative loss of the X-ray gas within the cooling radius (= 0.002 - 2.2 keV per particle), and apparently exceeds the energy required to cause the scaling relations to deviate from the self-similar predictions (=0.2 - 1.0 keV per particle). In contrast to the AGN feedback, the extra heating provided by supernova explosions accounts for = 0.01 - 0.08 keV per particle in groups and is almost negligible in clusters. Therefore, the observed correlation between △K0 and Lx can be considered as direct evidence for AGN feedback in galaxy groups and clusters.展开更多
The aim of this study was to highlight the effect of tide on the variation of the physicochemical parameter in the Kienké estuary. Six (06) environmental variables were monitored at nine (09) stations with the ti...The aim of this study was to highlight the effect of tide on the variation of the physicochemical parameter in the Kienké estuary. Six (06) environmental variables were monitored at nine (09) stations with the time step of one hour from 7 am to 7 pm on 4th</sup> August 2019. The hovmuller analysis showed that salinity, conductivity, total dissolved solids, and pH values increased during the flood phase and decreased during the ebb phase while oxygen concentration decreased during the flood and increased during the ebb phase. The stratification parameter has shown that the influx of seawater during high tide shifts the Kienké estuary from a well-mixed to a partially mixed environment.展开更多
In this paper we study some van den Bergh open clusters combining photometry and astrometry. A model which analyses the proper motion distribution and the stellar density is applied to find the kinematic parameters an...In this paper we study some van den Bergh open clusters combining photometry and astrometry. A model which analyses the proper motion distribution and the stellar density is applied to find the kinematic parameters and stellar membership in the region of the open clusters vdB92, vdB146 (NGC 7129) and vdB150. The astrometric data are obtained from UCAC4 catalogue. The centre coordinates, the components of mean proper motion, the angular diameter and the astrometric members are reported, taking the following values: for vdB92: α=105.97281°±0.13113°, δ=−11.57814°±0.10575°,?μαcosδ=−3.46±0.19mas/yr,μδ=1.27±0.19mas/yr, 34', 60 members;for vdB146: α=325.78423°±0.15297°, δ=66.13575°±0.02907°, μαcosδ=−2.71±0.25mas/yr, μδ=−3.32±0.25mas/yr, 9', 5 members;and for vdB150: α=332.22519°±0.06074°, δ=73.40232°±0.0.07789°, μαcosδ=3.07±0.90mas/yr, μδ=4.65±0.90mas/yr, 15', 7 members. The incidence of the proper motion errors in the determination of the cluster parameters and of the stellar membership is analysed and it is found that they do not significantly change. We finally compare the astrometric members with the photometric ones given in the literature.展开更多
Currently, land resources are becoming more and more constrained and structures are getting closer to each other. To investigate the seismic response of inter-story isolated structure to adjacent structure, models con...Currently, land resources are becoming more and more constrained and structures are getting closer to each other. To investigate the seismic response of inter-story isolated structure to adjacent structure, models considering no soil-structure interaction (SSI), considering soil-structure interaction (SSI), and considering structure-soil-structure interaction (SSSI) were established. Nonlinear seismic response comparative analysis was conducted by varying the spacing between adjacent structure and inter-story isolated structure, as well as the weight of adjacent structure, under different earthquake inputs, in order to obtain the structural response characteristics. The results indicate that the inter-story drift and inter-story shear of the inter-story isolated structure without considering SSI are smaller than those considering SSI and SSSI. The inter-story drift and inter-story shear of the inter-story isolated structure considering SSSI are further affected compared to that of the inter-story isolated structure considering only SSI. As the spacing between adjacent structure and inter-story isolated structure increases, the influence of adjacent structure on inter-story isolated structure decreases. The variation in the spacing between the two structures has a negligible effect on the isolation layer of the inter-story isolated structure. With the increase in the weight of adjacent structure, the influence of adjacent structure on inter-story isolated structure becomes more significant. The increasing weight of adjacent structure has an increasing effect on the Isolation layer of the inter-story isolated structure.展开更多
A new method for establishing ES cell lines from 129/ter、C57BL/6J mice was set up which was characterized by the murine embryonic fibroblast cell(MEF) feeder, the medium of rat heart cell-conditioned medium(RH-CM)for...A new method for establishing ES cell lines from 129/ter、C57BL/6J mice was set up which was characterized by the murine embryonic fibroblast cell(MEF) feeder, the medium of rat heart cell-conditioned medium(RH-CM)for ES cells, and the consecutive digestion by the digestion liquid containing 1% serum. Every group of improved experiments was done with a control of routine method. The results showed that, compared with routine method, the improved way increased the ratio of ES cell lines of 129/ter mice from 11.8% to 33.3%, and of C57BL/6J from 3.7% to 13.3%. The difference is distinct. The passage culture of ES cells showed that, compared with medium added LIF, RH-CM not only inhibited the differentiation of murine ES cells, maintained its dipoild karyotype, but also promote its adherence growth. This kind of culture condition not only maintained the ES cells in an undifferentiated state and their normal dipoild karyotype, but also a series of other characteristics of totipotent embryonic stem cells during extended culture period.展开更多
目的:通过检测Ter细胞在不同发病阶段胶原诱导性关节炎(collagen-induced arthritis,CIA)小鼠脾脏中的数量变化及高峰期CIA小鼠脾脏Ter细胞与关节评分和T、B细胞亚群比例的相关性,探讨Ter细胞在CIA发生和发展中的作用,从而进一步深入理...目的:通过检测Ter细胞在不同发病阶段胶原诱导性关节炎(collagen-induced arthritis,CIA)小鼠脾脏中的数量变化及高峰期CIA小鼠脾脏Ter细胞与关节评分和T、B细胞亚群比例的相关性,探讨Ter细胞在CIA发生和发展中的作用,从而进一步深入理解类风湿关节炎的发病机制。方法: 6~8周的DBA/1小鼠进行CIA模型的诱导,二次免疫后开始对CIA小鼠进行关节评分。根据发病时间和关节评分将CIA分为发病早期、高峰期、晚期三个阶段。发病高峰期小鼠根据最终关节评分再分为高评分组(>8分)和低评分组(≤8分),流式细胞术检测na ve小鼠和各个阶段CIA小鼠脾脏中Ter细胞比例及发病高峰期CIA小鼠脾脏T、B 细胞亚群比例,并进行关联分析。结果:发病高峰期CIA小鼠脾脏Ter细胞比例较na ve小鼠明显升高(8.522%±2.645% vs . 1.937%±0.725%, P < 0.01),高评分组小鼠脾脏Ter细胞比例明显低于低评分组(6.217%±0.841% vs . 10.827%±0.917%, P < 0.01 )。高评分组小鼠脾脏Th1细胞比例明显高于低评分组(1.337%±0.110% vs . 0.727%±0.223%, P < 0.05 ),高评分组小鼠脾脏Th17细胞比例高于低评分组(0.750%±0.171% vs . 0.477%±0.051%, P =0.099),高评分组小鼠脾脏生发中心B(germinal center B,GC-B)细胞比例明显高于低评分组(1.243%±0.057% vs . 1.097%±0.015%, P < 0.05 )。相关性分析结果显示,发病高峰期CIA小鼠脾脏Ter细胞比例与CD4 + T、Th1、Th17、GC-B细胞比例均呈强负相关,与B10细胞比例呈强正相关,相关性均有统计学意义,提示这群细胞在CIA中可能具有保护作用。动态变化研究显示,随着疾病进展,发病晚期CIA小鼠脾脏Ter细胞比例较高峰期明显降低(0.917%± 0.588% vs . 8.522%±2.645%, P <0.001),进一步提示这群细胞在关节炎中的保护作用。结论: Ter细胞在发病高峰期CIA小鼠脾脏中明显增加,与小鼠关节评分及致病性免疫细胞比例呈负相关,与保护性免疫细胞比例呈正相关,发病晚期CIA小鼠Ter细胞比例明显降低,提示Ter细胞可能作为一种保护性细胞参与类风湿关节炎的发生和发展,但其具体作用及机制仍需后续进一步的体内及体外实验验证。展开更多
基金Supported by National Key Technology R&D Program Project in the 12~(th) Five-Year Plan:The 3~(rd) Hunan Special Project of Grain Bumper Science and Technology "The Integration and Demonstration of High-yield,Water-saving and Fertilizer-saving Techniques in the South Rice Area of Middle Reaches of Yangtze"(2013BAD07B11)Agro-scientific Research Programs in Public Interest "Study on the Change of Soil Fertility and Fertility Techniques in the Major Grain Producing Areas and the Demonstration"(201203030)International Cooperation Project"Study on the Efficient Nutrient Management Technology of Modern Double Cropping Rice in Hunan Province"(IPNI Hunan-18)~~
文摘In order to study the effects of controlled release nitrogen fertilizer (CRNF) application on rapeseed, a simulated experiment was carried out with 3 types of paddy soils in Dongting Lake area for 4 consecutive years of applying CRNF under double rice cropping system after planting rapeseed crop in the fallow season. The effects of CRNF application on rapeseed yield, agronomic characters and soil fertility were studied in this paper. The results showed that CRNF application improved the growth of rapeseed plant and increased rapeseed yield of CRNF treatments in the purple calcareous clayed paddy soil (PCS) and alluvial loamy paddy soil (ALS) which respectively increased by 12.2% and 9.8% compared with applying urea, re- spectively. The rapeseed yield in 70% CRNF treatment obviously decreased com- pared with urea treatment. The contents of available N and organic carbon in soil increased by 25.0% and 3.2% in CRNF treatment in the ALS after rapeseed crop, respectively; and available N increased by 13.5% in the PCS. Both rapeseed yield and soil fertility in CRNF treatment and 70% CRNF treatment were lower than those in CK treatment in the reddish yellow clayed paddy soil (RYS). The results al- so indicated that the functions of CRNF application on rapeseed yield increase and soil nitrogen fertility improvement were very obvious in the PCS and ALS.
文摘Your comments are welcome!Please feel free to contact us with your personal stories or vivid pictures!Address:24 Baiwanzhuang St., Xicheng Dist., Beijing,100037E-mail:chinatodaynews@aliyun.com.
基金Supported by the National Natural Science Foundation of China(Grant Nos.10673008,10878001 and 10973010)the Ministry of Science and Technology of China(Grant No.2009CB824900/2009CB24904)the Ministry of Education of China(the NCET Program)
文摘By analyzing Chandra X-ray data of a sample of 21 galaxy groups and 19 galaxy clusters, we find that in 31 sample systems there exists a significant central (R ≤ 10 h^-171 kpc) gas entropy excess (AK0), which corresponds to = 0.1 - 0.5 keV per gas particle, beyond the power-law model that best fits the radial entropy profile of the outer regions. We also find a distinct correlation between the central entropy excess △K0 and K-band luminosity LK of the central dominating galaxies (CDGs), which is scaled as △K0 ∝ L K 1.6±04, where LK is tightly associated with the mass of the supermassive black hole hosted in the CDG. In fact, if an effective mass-to-energy conversionefficiency of 0.02 is assumed for the accretion process, the cumulative AGN feedback E AGN feedack=ηMBHc2 yields an extra heating of = 0.5 - 17.0keV per particle, which feedback is sufficient to explain the central entropy excess. In most cases, the AGN contribution can compensate the radiative loss of the X-ray gas within the cooling radius (= 0.002 - 2.2 keV per particle), and apparently exceeds the energy required to cause the scaling relations to deviate from the self-similar predictions (=0.2 - 1.0 keV per particle). In contrast to the AGN feedback, the extra heating provided by supernova explosions accounts for = 0.01 - 0.08 keV per particle in groups and is almost negligible in clusters. Therefore, the observed correlation between △K0 and Lx can be considered as direct evidence for AGN feedback in galaxy groups and clusters.
文摘The aim of this study was to highlight the effect of tide on the variation of the physicochemical parameter in the Kienké estuary. Six (06) environmental variables were monitored at nine (09) stations with the time step of one hour from 7 am to 7 pm on 4th</sup> August 2019. The hovmuller analysis showed that salinity, conductivity, total dissolved solids, and pH values increased during the flood phase and decreased during the ebb phase while oxygen concentration decreased during the flood and increased during the ebb phase. The stratification parameter has shown that the influx of seawater during high tide shifts the Kienké estuary from a well-mixed to a partially mixed environment.
文摘In this paper we study some van den Bergh open clusters combining photometry and astrometry. A model which analyses the proper motion distribution and the stellar density is applied to find the kinematic parameters and stellar membership in the region of the open clusters vdB92, vdB146 (NGC 7129) and vdB150. The astrometric data are obtained from UCAC4 catalogue. The centre coordinates, the components of mean proper motion, the angular diameter and the astrometric members are reported, taking the following values: for vdB92: α=105.97281°±0.13113°, δ=−11.57814°±0.10575°,?μαcosδ=−3.46±0.19mas/yr,μδ=1.27±0.19mas/yr, 34', 60 members;for vdB146: α=325.78423°±0.15297°, δ=66.13575°±0.02907°, μαcosδ=−2.71±0.25mas/yr, μδ=−3.32±0.25mas/yr, 9', 5 members;and for vdB150: α=332.22519°±0.06074°, δ=73.40232°±0.0.07789°, μαcosδ=3.07±0.90mas/yr, μδ=4.65±0.90mas/yr, 15', 7 members. The incidence of the proper motion errors in the determination of the cluster parameters and of the stellar membership is analysed and it is found that they do not significantly change. We finally compare the astrometric members with the photometric ones given in the literature.
文摘Currently, land resources are becoming more and more constrained and structures are getting closer to each other. To investigate the seismic response of inter-story isolated structure to adjacent structure, models considering no soil-structure interaction (SSI), considering soil-structure interaction (SSI), and considering structure-soil-structure interaction (SSSI) were established. Nonlinear seismic response comparative analysis was conducted by varying the spacing between adjacent structure and inter-story isolated structure, as well as the weight of adjacent structure, under different earthquake inputs, in order to obtain the structural response characteristics. The results indicate that the inter-story drift and inter-story shear of the inter-story isolated structure without considering SSI are smaller than those considering SSI and SSSI. The inter-story drift and inter-story shear of the inter-story isolated structure considering SSSI are further affected compared to that of the inter-story isolated structure considering only SSI. As the spacing between adjacent structure and inter-story isolated structure increases, the influence of adjacent structure on inter-story isolated structure decreases. The variation in the spacing between the two structures has a negligible effect on the isolation layer of the inter-story isolated structure. With the increase in the weight of adjacent structure, the influence of adjacent structure on inter-story isolated structure becomes more significant. The increasing weight of adjacent structure has an increasing effect on the Isolation layer of the inter-story isolated structure.
文摘A new method for establishing ES cell lines from 129/ter、C57BL/6J mice was set up which was characterized by the murine embryonic fibroblast cell(MEF) feeder, the medium of rat heart cell-conditioned medium(RH-CM)for ES cells, and the consecutive digestion by the digestion liquid containing 1% serum. Every group of improved experiments was done with a control of routine method. The results showed that, compared with routine method, the improved way increased the ratio of ES cell lines of 129/ter mice from 11.8% to 33.3%, and of C57BL/6J from 3.7% to 13.3%. The difference is distinct. The passage culture of ES cells showed that, compared with medium added LIF, RH-CM not only inhibited the differentiation of murine ES cells, maintained its dipoild karyotype, but also promote its adherence growth. This kind of culture condition not only maintained the ES cells in an undifferentiated state and their normal dipoild karyotype, but also a series of other characteristics of totipotent embryonic stem cells during extended culture period.
文摘目的:通过检测Ter细胞在不同发病阶段胶原诱导性关节炎(collagen-induced arthritis,CIA)小鼠脾脏中的数量变化及高峰期CIA小鼠脾脏Ter细胞与关节评分和T、B细胞亚群比例的相关性,探讨Ter细胞在CIA发生和发展中的作用,从而进一步深入理解类风湿关节炎的发病机制。方法: 6~8周的DBA/1小鼠进行CIA模型的诱导,二次免疫后开始对CIA小鼠进行关节评分。根据发病时间和关节评分将CIA分为发病早期、高峰期、晚期三个阶段。发病高峰期小鼠根据最终关节评分再分为高评分组(>8分)和低评分组(≤8分),流式细胞术检测na ve小鼠和各个阶段CIA小鼠脾脏中Ter细胞比例及发病高峰期CIA小鼠脾脏T、B 细胞亚群比例,并进行关联分析。结果:发病高峰期CIA小鼠脾脏Ter细胞比例较na ve小鼠明显升高(8.522%±2.645% vs . 1.937%±0.725%, P < 0.01),高评分组小鼠脾脏Ter细胞比例明显低于低评分组(6.217%±0.841% vs . 10.827%±0.917%, P < 0.01 )。高评分组小鼠脾脏Th1细胞比例明显高于低评分组(1.337%±0.110% vs . 0.727%±0.223%, P < 0.05 ),高评分组小鼠脾脏Th17细胞比例高于低评分组(0.750%±0.171% vs . 0.477%±0.051%, P =0.099),高评分组小鼠脾脏生发中心B(germinal center B,GC-B)细胞比例明显高于低评分组(1.243%±0.057% vs . 1.097%±0.015%, P < 0.05 )。相关性分析结果显示,发病高峰期CIA小鼠脾脏Ter细胞比例与CD4 + T、Th1、Th17、GC-B细胞比例均呈强负相关,与B10细胞比例呈强正相关,相关性均有统计学意义,提示这群细胞在CIA中可能具有保护作用。动态变化研究显示,随着疾病进展,发病晚期CIA小鼠脾脏Ter细胞比例较高峰期明显降低(0.917%± 0.588% vs . 8.522%±2.645%, P <0.001),进一步提示这群细胞在关节炎中的保护作用。结论: Ter细胞在发病高峰期CIA小鼠脾脏中明显增加,与小鼠关节评分及致病性免疫细胞比例呈负相关,与保护性免疫细胞比例呈正相关,发病晚期CIA小鼠Ter细胞比例明显降低,提示Ter细胞可能作为一种保护性细胞参与类风湿关节炎的发生和发展,但其具体作用及机制仍需后续进一步的体内及体外实验验证。