研究隐伏断裂的一种新方法——跨断裂地面光谱测量的应用

1989年和1990年,利用地物光谱仪对南口-孙河隐伏断裂进行了8条测线光谱反射率重复测量,并对各种影响因素予以详细分析。结果表明:(1)断裂两侧光谱反射率明显不同,上升盘的反射率高于下降盘;(2)时隔一年的原测线重复测量结果显示,断裂两侧光谱反射率的相对值有所变化。这表明本方法不但可以确定断裂有无及性质。而且可通过重复测量来分析断裂的活动特征。根据测量结果,认为南口-孙河断裂的具体位置应向北移,西断裂的东端可能在百善附近,未向东继续延伸。东断裂的最新活动似乎比西断裂强。     

海洋光谱测量与数据分析处理方法

海洋水色遥感的基础之一是海洋光谱特性的精确测量与分析。海洋光谱分析对改进反演算法、最佳波段选择、辅助大气修正、系统定标与校验等方面有很大作用,因此为方面的研究越来越受到重视。本文在海洋光谱机理的基础上,就光谱现场测量方法和分析处理方法进行了探讨,并给出一个典型海域的史谱数据分析处理结果。由于我国尚缺乏满足水色应用要求和水下光学测量仪器,因此提出了一种利用瞬态光谱仪在水面以上进行离水辐射率测量与分析     

海洋高光谱实时观测技术系统简介

“海洋高光谱实时观测技术系统”是由中国科学院南海海洋研究所等单位完成的国家“863”计划“海洋光学浮标技术”课题的一项重要成果。该技术系统主要包括海洋光学浮标总体集成技术、浮标设计技术、浮标平台对水下光辐射测量阴影效应模拟技术、海面入射太阳光谱辐照度高光谱测     

西沙群岛附近海域船舶尾迹水体遥感反射率特性的实验测量与分析

利用海上实验现场测量船舶的尾迹气泡群对西沙群岛附近海域一类水体海水光学特征(例如归一化离水辐亮度、遥感反射率)的影响,为通过星载光学传感器遥感获取船舶尾迹信息提供理论依据。实验证明,在可见光和近红外波段,船舶含气泡尾迹不仅在幅度上、也在谱形上改变海水遥感反射率,作为结果,尾迹气泡使得海水变得更绿;同时,随着观测点在尾迹中的位置距目标船的接近,气泡密度不断增大,反射率也随之增强。     

水面之上法测量水体光谱的关键技术

对水体光谱特征的研究是海洋水色遥感的基础工作之一。水体的光谱特征包括:表观光学特性和固有光学特性。在水体的表观光学特性研究方面,目前国际水色界推行的有:剖面法和水面之上法(也称表面法)。由于我国近岸水体混浊度较高,浅水区域较多,研究这类水体的表观光学特性应以水面之上法为主、剖面法为辅。介绍了水面之上法水体光谱的测量技术,就其中关键技术问题进行了讨论。     

Measurements of ocean wave spectrum from airborne radar at small incidence angles

This paper proposes the retrieval method of ocean wave spectrum for airborne radar observations at small incidence angles, which is slightly modified from the method developed by Hauser. Firstly, it makes use of integration method to estimate total mean square slope instead of fitting method, which aims to reduce the affects of fluctuations superposed on normalized radar cross-section by integration. Secondly, for eliminating the noise spectrum contained in signal spectrum, the method considers the signal spectrum in certain look direction without any long wave components as the assumed noise spectrum, which would be subtracted from signal spectrum in any look direction for linear wave spectrum retrieval. Estimated ν from the integration method are lower than the one from fitting method and have a standard deviation of 0.004 between them approximately. The assumed noise spectrum energy almost has no big variations along with the wave number and is slightly lower to the high wave number part of signal spectrum in any look direction, which follows that the assumption makes sense. The retrieved directional spectra are compared with the buoy records in terms of peak wavelength, peak direction and the significant wave height. Comparisons show that the retrieved peak wavelength and significant wave height are slightly higher than the buoy records but don’t differs significantly (error less than 10%). For peak direction, the swell waves in first case basically propagate in the wind direction 6 hours ago and the wind-generated waves in second case also propagate in the wind direction, but the 180? ambiguity remains. Results show that the modified method can carry out the retrieval of directional wave spectrum.     

第十三届国际天文与天体物理奥林匹克竞赛实测试题

1.新星海豚座2013的测光与光谱2013年8月14日1401 UT(MJD=56518.584)Koichi hagaki发现了星等为6.8的经典新星海豚座V339(海豚座新星 2013)。专业和业余天文学家很快开始了新星的测光和光谱测量消息发出后不到10小时,当匈牙利夜幕降临时,当地天文学家使用1m望远镜接eShel echelle光谱仪拍摄了该新星的第—条光谱。根据图1.1和12回答以下问题。     

Measurement of the current and spectral analysis on the continental shelf in the East China Sea

Direct measurements of current velocity and water temperature were undertaken at the mooring Sta. M (125°29.38' N, 31°49.70' E) on the continental shelf area in the East China Sea in June 1999 by R/V Xiangyanghong 14. The relationship between various time series of oceanic fluctuations is calculated by spectral analysis. The major results are as follows: (1) an average (u,v) of (6.9,-3.0 cm/s) at the 30 m depth is obtained during the 9-day observation, and that at the 45 m depth is (3.7,-1.1 cm/s), i. e., the mean flows are southeastward at both the 30 and 45 m depths;the currents become stronger gradually during the observation period; this may be mainly attributed to the transition of the tidal currents from neap to spring; (2)semidiurnal fluctuation is the most dominant in the current fluctuations, and rotates mainly clockwise; in the next place, there is also diurnal fluctuation;the local inertial period is close to the period of diurnal fluctuation, and an inertial motion is clockwise; thus, loca     

A Kinetic Spectrophotometric Method for the Determination of Iron （Ⅲ） in Water Samples

A new kinetic spectrophotometric method has been developed for the determination of iron (Ⅲ). The method is based on the catalytic effect of iron (Ⅲ) on the oxidation of weak acid brilliant blue dye (RAWL) by KIO4 in acid medium. The advantages of the proposed method are that it is sensitive, accurate, rapid, inexpensive, can be operated under room temperature and has a large determination concentration range compared to other techniques. The obtained optimum conditions are pH 3.15, RAWL (200 mgL-1) 5.00mL, Potassium periodate solution (0.01 molL-1) 0.30mL, phenanthroline (0.02molL-1) 1.00mL, reaction temperature 25℃ and reaction time 7 miu. With this method iron could quantitively be determined in the range 0.00-0.02 mgL-1, the detection limit being 4.10×10-10mL-1. The relative standard deviations (RSD) in five replicate determinations for 3 μgL-1 and 5μgL-1 iron (Ⅲ) are 3.1% and 1.9%, respectively. The method has been applied to the determination of iron (Ⅲ) in tap water samples and seawater samples (from the South China Sea), the recovery rates being 98.0% and 100.5%, respectively.     

船舶含气泡尾迹的光学特性研究

基于充分挖掘卫星遥感应用于海洋监测能力的需求,通过海上试验测量船舶含气泡尾迹海水的物理、光学特征,研究气泡群对不同水体光学特征的影响,例如离水辐亮度、遥感反射率.这些工作可为通过星载光学传感器遥感获取船舶尾迹信息提供理论依据.试验证明在可见光和近红外波段船舶含气泡尾迹相对于背景海水的离水辐亮度、遥感反射率都不同程度地得到了增强,并且在一类水体中含气泡尾迹的光谱后向散射无论是相对增幅还是绝对增幅都要远大于二类水体中的.