内蒙古农牧交错区农耕地土壤风蚀规律的风洞试验研究

该研究采用室内风洞试验,在不同风速、坡度及土壤含水量条件下,对两种不同质地土壤的风蚀规律进行了研究。研究结果表明,土壤风蚀量随风速的增加而增加,并存在临界风速,当风速大于此临界值时风蚀量急剧增加,但土壤的质地不同,其风蚀量增大的幅度亦不相同;同时两种土壤的风蚀量存在临界坡度,当吹蚀坡度超过此临界值时风蚀量随着坡度的变化又增加变为减少,壤土的临界坡度为20°,砂壤土10°。增加土壤含水量可以显著降低土壤的风蚀量,对于扰动土,壤土和砂壤土均存在一个5%的临界土壤含水量,当土壤含水量大于临界值时,两者的风蚀量随着含水量的增加而减少的程度明显增强,且壤土的风蚀量总体上高于砂壤土。对于未扰动土,壤土和砂壤土的风蚀量随土壤含水量的降低而增加的趋势均不明显,特别是对于壤土,当土壤含水量相同时扰动土的风蚀量明显大于未扰动土的风蚀量,说明减少表层土壤的扰动可以显著抑制土壤风蚀的强度

LABORATORY STUDY ON SEDIMENT TRANSPORT CAPACITY IN THE DYNAMIC PROCESS OF RILL EROSION

细沟水流的输沙能力是土壤侵蚀的重要参数之一,对于土壤侵蚀预报和土壤侵蚀过程模拟尤为重要。在不考虑土壤团粒结构条件下,根据集中稳定水流条件下侵蚀产沙随沟长增加而增加并将最终趋近于水流输沙能力的事实,提出了通过改变沟长来量测水流输沙能力的实验室水槽测量方法。相应地提出了根据试验数据计算水流输沙能力的函数表达式。用一种粉粘（黄土）土壤,进行了一系列（405次）室内水槽摹拟试验。采用五种坡度（5°,10°,15°,20°,25°）、三个流量（2,4,8 L min-1）的细沟侵蚀产沙数据,分析了输沙能力与沟坡、入流量的相互关系

2005～2015年CERN光合有效辐射数据集

光合有效辐射在生态学、农学以及气候学等多个学科中都有重要的应用价值。它是揭示物质与能量交换过程的基本生理变量,是光合潜力、潜在产量的评估研究和作物生长模拟研究、土壤碳的固定模拟研究中不可缺少的关键数据之一。该数据集涵盖了中国8个典型陆地生态类型、中国生态系统研究网络(CERN)下属的40个辐射观测站观测的光合有效辐射日均值,时间跨度为2005～2015年。通过对传感器的集中标定与规范的数据质量控制方案,保障了观测数据的可靠性与可比性。采用光谱仪、辐射标准灯传递辐射基准方案,对光合有效辐射传感器进行集中标定与比对,标定精度小于5%,符合世界气象组织(WMO)标准;采用极值法对观测的光合有效辐射数据进行质量控制

JUNO Sensitivity on Proton Decay p→νˉK+p\to \bar\nu K^+ Searches

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this paper, the potential on searching for proton decay in $p\to \bar\nu K^+$ mode with JUNO is investigated.The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits to suppress the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar\nu K^+$ is 36.9% with a background level of 0.2 events after 10 years of data taking. The estimated sensitivity based on 200 kton-years exposure is $9.6 \times 10^{33}$ years, competitive with the current best limits on the proton lifetime in this channel

JUNO sensitivity on proton decay p → ν K + searches*

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this study, the potential of searching for proton decay in the $p\to \bar{\nu} K^+$ mode with JUNO is investigated. The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits suppression of the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar{\nu} K^+$ is 36.9% ± 4.9% with a background level of $0.2\pm 0.05({\rm syst})\pm$$0.2({\rm stat})$ events after 10 years of data collection. The estimated sensitivity based on 200 kton-years of exposure is $9.6 \times 10^{33}$ years, which is competitive with the current best limits on the proton lifetime in this channel and complements the use of different detection technologies