一种复杂海天背景下的红外舰船目标自动检测方法

提出了一种红外舰船目标检测算法。首先,利用设计好的频域组合高通滤波器对原始红外图像进行处理,以得到舰船目标可能存在的区域即目标潜在区;然后,对获得的目标潜在区进行尺度自适应的局部阈值分割,进而提取出较为完整的舰船目标或者虚假目标;最后通过检测吃水线特征来筛选出正确的舰船目标。实验结果表明,此算法能够有效地检测出复杂海天背景条件下的红外舰船目标,且具有一定的时效性。     

风廓线雷达资料在台风苏拉登陆过程中的应用初探

为了研究风廓线雷达在台风天气过程预报中的作用,对2012年8月2—4日在福建秦屿镇登陆的台风苏拉天气过程统计分析,结果表明：风廓线雷达在台风苏拉登陆期间4 km以上高空有效数据获取率明显提高,确定风廓线雷达的有效探测高度为4.8 km;通过信噪比和垂直速度数据统计分析出台风登陆前后带来间歇性的降雨,而台风眼登陆主要表现为无降水天气,仅有少量的降雨,这一结论进一步在小时降雨量统计中得到验证;通过水平风速数据统计分析出台风登陆前后在有效探测高度内水平风速在25 m·s-1左右,而台风眼登陆水平风速在0~3 m·s-1; 统计结果与台风登陆物理过程相吻合。     

The Influences of Various Factors and Interest Demands on Linpan Landscape Evolution in the Chengdu Plain: A Qualitative Study based on Oral Histories

Traditional rural homegarden agroforestry systems in the Chengdu Plain of China are often referred to as “Linpan” in Chinese, which integrates the landscape of ecological functions and human production activities. In recent years, due to the influences of urbanization and the aging population, the Linpan landscape has changed dramatically. Clarifying the factors which influence Linpan landscape evolution is a critical way to improve rural landscape renovation. Through oral history interviews, the deep-seated factors driving the evolution of the Linpan landscape form from 1949 to 2020 are explored using the grounded theory. The results show that in the process of Linpan landscape evolution, beneficiary groups, the material basis, and cultural characteristics are the prerequisites for changing the Linpan settlement landscape. The demand of production and life and government-led behavior are the two main influencing factors, and landscape change is the final result. The demand of production and life from the residents is the primary internal driving force of landscape change, while government-led behavior is the main external driving force of settlement development and evolution. The nature of the main driving forces behind the evolution of the Linpan landscape in the Chengdu Plain can be divided into three stages. (1) From 1949 to 1980, it was characterized as a balancing of government forces and social forces. (2) From 1981 to 1993, it was characterized by social forces suppressing government forces. (3) From 1994 to 2020, it was characterized as a stalemate between the government and social forces. From the perspective of the evolution of the Linpan settlement landscape, the traditional Linpan form and settlement layout have been unable to meet the new requirements of the rural social and economic transition period. They are facing the challenges of rural reconstruction and rural revitalization. In the future, village and town planning and the design of new settlements need to comprehensively consider the demands of different interest groups.     

Distribution of phosphine in the offshore area of the Southwest Yellow Sea,East Asia

Phosphine is a natural gaseous compound in the phosphorus biogeochemical cycle. This paper studies the spatial and temporal distributions of matrix-bound phosphine (MBP) and gaseous phosphine in the offshore area of the Southwest Yellow Sea, East Asia. The results show that MBP concentrations in marine surface sediments range from 0.69 ± 0.06 ng/kg (dry) to 179 ± 29 ng/kg (dry). Higher seasonal MBP concentrations in sediments are found in fall than in spring or winter in most sites. High MBP contents are observed in two fish-breeding areas. MBP concentrations decrease with distance to the coast, except in the southeast of the sampling area. MBP levels in marine sediments are found to be higher than those at several other places: freshwater sediments and soil, except eutrophic lakes. Gaseous phosphine contents in fall range from 0.14 ± 0.00 ng/m³ to 9.83 ± 0.97 ng/m³. No correlation is observed between MBP and gaseous phosphine.     

基于遥感与GIS的矿山地质环境时空演变分析——以东胜矿区为例

煤矿开采将不可避免地产生地质环境问题。以东胜矿区2007年Quick Bird遥感影像和2012年World View2影像为数据源,通过提取矿山地质环境现状信息,计算矿山地质环境类型时空数据的变化幅度、变化速度及转移矩阵等,揭示不同矿山地质环境类型的时间变化过程;以采矿权为空间单元,通过计算各类矿山地质环境的年均增幅与综合动态度,描述其空间演变趋势。结果表明:随着东胜矿区开采规模持续扩大,不同矿山地质环境类型的面积逐年增加且增幅各异,由"污染"(采坑、排土场及积水区)向"治理"(恢复治理区和工业广场)转移的趋势显著;尽管矿区地质环境已得到足够重视,并呈现西北区域恢复治理优于东南区域的特点,但"治理"力度总体上慢于"污染"程度,仍不利于可持续发展。     

广西资源县某萤石矿矿山地质灾害危险性评估及防治对策

以广西资源县某萤石矿山为例,重点介绍矿山地质灾害危险性评估的分析思路及基本方法,并提出有效的防控对策。在了解矿山基本情况和查明矿山地质环境背景的基础上,综合采矿场地形及工程活动特征,对矿山地质灾害进行现状评估和预测评估,并提出了相应的防治对策。     

Implementation of New OPAL Tables in Eggleton's Stellar Evolution Code

Based on previous works of OPAL, we construct a series of opacity tables for various metallicities Z=0, 0.000 01, 0.000 03, 0.000 1, 0.000 3, 0.001, 0.004, 0.01, 0.02, 0.03, 0.04, 0.05, 0.06, 0.08 and 0.1. These tables can be easily used in Eggleton's stellar evolution code in place of the old tables without changing the code. The OPAL tables are used for log10(T/K) > 3.95 and Alexander's for log10(T/K) < 3.95. At log10(T/K) = 3.95, the two groups' data fit well for all hydrogen mass fractions. Conductive opacities are included by reciprocal addition according to the formulae of Yakovlev and Urpin. A comparison of 1 and 5 M models constructed with the older OPAL tables of Iglesias and Rogers shows that the new opacities have most effect in the late stages of evolution, the extension of the blue loop during helium burning for intermediate-mass and massive stars.     

广西1999年12月严重霜冻与典型霜冻重年的环流对比分析

通过对1999年12月广西严重霜冻天气同期500hPa高度场和海平面气压场特征及前期500 hPa高度的相关场分析,得到北半球中高纬度槽脊的位置与强度,地面大陆冷高压强弱,是影响广西12月霜冻的主要环流形势;当年1月、9月极涡强度、位置,北美高压脊强度,及黑海附近低槽强弱,是影响广西12月霜冻天气重、轻的重要因子。     

Optical Photometric Observations of 7-Ray Loud Blazars

We report results of our optical photometric observations of ten gamma-ray loud blazers, namely: 0219+428 (3C66A), PKS 0420-014 (OA 129), S5 0716+714, 0754+100 (OI 090.4), 0827+243 (OJ248), 1652+398 (Mrk 501), 2200+420 (BL Lacertae), 2230+114 (CTA 102), 2251+158 (3C 454.3) and 2344+514. The observations were carried out in September-October, 2000 using the 70 cm optical telescope at Abstumani Observatory, Georgia. We found intra-day variations in 0420-014, S5 0716+714, BL Lacertae and CTA 102. A variation of 0.3 magnitude over a time scale of about 3 hours was observed in the R passband in BL Lacertae on JD 2451827. We did not detect any variation in 3C 66A, Mrk 501, or 3C 454.3 during our observations. Nor did we detect any clear evidence of variation in 1ES 2344+514 during our two weeks' observing run of the TeV gamma-ray source.