一种基于亮度调制的多源遥感影像融合方法

分析了基于亮度调制的多源遥感影像融合方法,利用HIS变换和àtrous小波变换,根据逐步对亮度分量进行调制的思想,实现了武汉城郊地区SPOT、TM和ENVISAT SAR影像的融合,使融合影像在保持光谱信息、提高空间分辨率和增强纹理信息方面取得了较好的效果,有利于目标判读和影像分类等后续处理.     

The global rainforest mapping project JERS-1:a paradigm of international collaboration for monitoring land cover change

The Global Rainforest Mapping (GRFM) project was initiated in 1995 and, through a dedicated data acquisition policy by the National Space Development Agency of Japan (NASDA), data acquisitions could be completed within a 1.5-year period, resulting in a spatially and temporally homogeneous coverage to contain the entire Amazon Basin from the Atlantic to the Pacific; Central America up to the Yucatan Peninsular in Mexico; equatorial Africa from Madagascar and Kenya in the east to Sierra Leone in the west; and Southeast Asia, including Papua New Guinea. To some extent, GRFM project is an international endeavor led by NASDA, with the goal of producing spatially and temporally contiguous Synthetic Aperture Radar (SAR) data sets over the tropical belt on the Earth by use of the JERS-1 L-band SAR, through the generation of semi-continental, 100m resolution, image mosaics. The GRFM project relies on extensive collaboration with the National Aeronautics and Space Administration (NASA), the Joint Research Center of the European Commission (JRC) and the Japanese Ministry of International Trade and Industry (MITI) for data acquisition, processing, validation and product generation. A science program is underway in parallel with product generation. This involves the agencies mentioned above, as well as a large number of international organizations, universities and individuals to perform field activities and data analysis at different levels.     

Effect of the Initial Vortex Structure on Intensity Change During Eyewall Replacement Cycle of Tropical Cyclones: A Numerical Study

This study investigates the effect of the initial tropical cyclone (TC) vortex structure on the intensity change during the eyewall replacement cycle (ERC) of TCs based on two idealized simulations using the Weather Research and Forecasting (WRF) model. Results show that an initially smaller TC with weaker outer winds experienced a much more drastic intensity change during the ERC than an initially larger TC with stronger outer winds. It is found that an initially larger TC vortex with stronger outer winds favored the development of more active spiral rainbands outside the outer eyewall, which slowed down the contraction and intensification of the outer eyewall and thus prolonged the duration of the concentric eyewall and slow intensity evolution. In contrast, the initially smaller TC with weaker outer winds corresponded to higher inertial stability in the inner core and weaker inertial stability but stronger filamentation outside the outer eyewall. These led to stronger boundary layer inflow, stronger updraft and convection in the outer eyewall, and suppressed convective activity outside the outer eyewall. These resulted in the rapid weakening during the formation of the outer eyewall, followed by a rapid re-intensification of the TC during the ERC. Our study demonstrates that accurate in- itialization of the TC structure in numerical models is crucial for predicting changes in TC intensity during the ERC. Additionally, monitoring the activity of spiral rainbands outside the outer eyewall can help to improve short-term intensity forecasts for TCs experiencing ERCs.     

1996-2022年黄河三角洲行水河口岸线稳定性研究

黄河清八汊现行河口自改汊以来发生了巨大变化,监测其岸线变化,探讨其稳定程度对海岸带可持续发展以及海岸带韧性评估具有重要意义。本研究利用GPS、GIS、RS技术从1996—2022年黄河三角洲行水河口的220幅遥感影像中推断出年平均海岸线位置,同时根据行水河口摆动次数划分为5个阶段,并以此为基础对海岸线变迁及其稳定性进行定量分析。结果表明：行水河口岸线长期处于动态变化过程中,整体呈淤进状态,各岸段岸线时空变化特征不同,最大侵蚀（-73.89m/a）区出现在两丁坝之间,最大淤积（393.20m/a）区出现在河口区附近。研究区90%的岸线表现为较强淤积至严重淤积,稳定性指数由两丁坝之间（0.135）、2007年出汊前旧河口（0.068）、2007年出汊后新生河口（0.006）依次降低。入海水沙量、河口位置变迁以及沿岸输沙是影响岸线稳定性出现时空差异的主要原因。     

基于红外探测器焦平面成像的白天测星技术研究

对于大气层以下的传统可见光天文导航,存在白天日照强烈而无法观测星体,数据缺乏连续性,可观测恒星数量少,无法实现全天时天文导航等问题。文中设计并探究利用红外探测器焦平面成像技术来取代可见光CCD成像技术的短波红外天文导航方法,分析短波红外波段相对于可见光波段,在大气层内白天观星实现全天时天文导航的优势,并对其可行性进行实验分析。实验结果表明,基于红外探测器的天文导航方法,在太阳辐射较弱的清晨或黄昏等时段,可以成功拍摄到可见光CCD仪器无法观测到的短波红外波段的恒星,对于实现全天时天文导航具有一定的参考意义。夜间短波红外波段的可供观测恒星数量远远多于可见光恒星数量,这对于增加多余观测量,保证连续测量输出,提高天文导航定位定向的精度,具有实际的应用价值。     

喀斯特山区溪流上覆水—孔隙水—沉积物中不同形态氮的赋存特征及其迁移——以麦西河为例

选取贵州百花湖入湖支流麦西河为对象,研究了上覆水—孔隙水—沉积物体系氮的形态差异,结果表明:麦西河上覆水中,以硝态氮(NO-3-N)为主,氨态氮(NH+4-N)次之,亚硝态氮(NO-2-N)最低;孔隙水中,溶解无机氮中以NH+4-N为主, NO-3-N次之, NO-2-N最低;沉积物中,总氮(TN)的含量为1110.67～4413.16mg/kg;固定态铵含量为34.56～170.05mg/kg,占TN的1.47%～6.25%;可交换态氮以NH+4-N为主, NO-3-N次之, NO-2-N最低。孔隙水NH+4-N是上覆水NH+4-N的2.65～19.51倍,上覆水NO-3-N是孔隙水NO-3-N的7.14～20.43倍。沉积物TN与孔隙溶解水无机氮(DIN)、孔隙水NH+4-N、沉积物可交换态氮和沉积物可交换性NH+4-N呈显著正相关;在沉积物中,可交换性NO-3-N与可交换性NH+4-N及可交换态氮呈显著正相关,可交换性NH+4-N与可交换态氮呈极显著正相关;孔隙水溶解无机氮与孔隙水NH+4-N呈极显著正相关。麦西河不同介质中氮的迁移关系则表现为:由于浓度梯度,上覆水中的NO-3-N扩散到孔隙水中,进而累积到沉积物中;沉积物的可交换性NH+4-N,进入孔隙水,最终扩散到上覆水中。      

贵州普定陈旗堡地区土体主要理化性质与持水量相关性研究

根据贵州普定陈旗堡典型喀斯特地区的生态特性,从水文地质与工程地质角度,借助土壤学对土壤水分特性的研究理论,对表层土壤20cm以下土层的土体物理化学性质与土体水分含量,即土体的持水量（waterholding capacity),进行了相关性研究。分析结果表明：土体颗粒成分、孔隙比、矿物成分含量等对土体水分含量均有影响。土体中粉粒含量较高而粘粒含量较少,且粒度分配不均匀时,土体水分含量相对较高;孔隙率高的土体水分含量较高;伊蒙混层矿物、伊利石和绿泥石等粘土矿物含量较高时,土体水分含量相对较高,而长石、碳酸盐等原生矿物含量较高时,土体水分含量相对较小。石英对于土体持水量影响不明显。     

面向对象的高分遥感影像信息提取技术研究

以World View-2高分遥感影像数据为例,采用规则集开发的模式进行地图要素提取,对主要制图要素图像进行了分割、分类试验,实现了多尺度分割的层次构建和制图地物要素分级分类。     

川西甲基卡烧碳沟地区伟晶岩脉地球化学特征

通过对烧碳沟地区伟晶岩的岩石学特征及地球化学特征进行分析,探讨了其成矿构造背景及物质来源等成矿地质条件.结果表明:烧碳沟一带伟晶岩的SiO2含量为73.46%~75.96%,全碱含量为4.71%~7.36%,里特曼指数为0.70~1.84,反映了伟晶岩的钙碱性特征;铝饱和指数A/CNK 为1.54~2.49,全部大于1.1,反映了强过铝质S 型花岗岩的特征.伟晶岩的主量、微量和稀土元素特征表明,其源岩以黏土沉积物为主,与甲基卡二云母花岗岩相比,两者具有高度相似的微量、稀土元素配分模式,以及近似的Nb/Ta 比值,表明两者具有同源性,且属于分异程度较高的钙碱性花岗伟晶岩脉.构造背景分析显示伟晶岩属于同碰撞花岗岩,在印支运动末期相对稳定的环境中,甲基卡一带的穹状构造为稀有金属伟晶岩矿床提供了良好的成矿环境.     

便携式Li-K分析仪的研制及其在锂辉石中锂的分析应用

我国锂钾主要矿产资源大多分布在西部偏远地区,其勘查找矿或综合利用迫切需要现场快速分析技术的支持。本文介绍了自行开发的便携式Li-K分析仪的主要性能及其在锂辉石中锂的分析应用。Li-K分析仪是一种基于大气压的液体阴极辉光放电光谱仪,以待测液体为放电阴极,实现了样品中Li、K等元素的原子化和激发。该仪器以光纤传导CCD光谱仪作为检测器,其波长范围为345~1015 nm,分辨率3 nm;以Li 670.78 nm和K 769.90 nm分析谱线,在仪器最佳工作条件下测定Li、K的精密度(RSD,n=14)均低于2%,检出限为0.03μg/m L,检测范围0.1~10μg/m L。研究表明,不同酸度和酸的类型对谱线强度影响较大,且存在显著的样品基体效应,标准曲线法分析锂辉石中Li的结果偏差高达267%;而标准加入法可克服基体效应的影响,获得与ICP-OES一致性较好的分析结果,为现场开展固体样品中Li的测定奠定了基础。