Summer Arctic sea fog     

Xie Simei  Xue Zhenhe  Jiang Dezhong  Zou Bin  Qu Shaohou 《海洋学报(英文版)》2001,20(2):183-196

I~IOXSea fog is a kind of dangerous weather. Chinese sea fog experts, Wang Binhua (1983),Hu Ruijin and Zhou Faxiu (1998) and Hu Jifu et al. (1996) studied sea fog rather Systematically. FOreign Experts also Paid great attention to sea fog. Ernlnons and Montgomery(1974), chipper (1994) and Rayrnond et al. (1989) have studied sea fog thorOUghly.HOwever, studies on Arctic sea ice have rarely been carried Out becauSe of the sever environment and less htnnan activity in the region. There …  相似文献   

海洋微藻多糖微波提取法研究   总被引：1，自引：0，他引：1  

刘四光  李文权  邓永智 《海洋通报》2007,26(4):105-110

选取自养小球藻(Chlorella autotrophica)为实验材料,采用微波法提取多糖,以温度、时间、pH以及微波功率4个因子建立正交实验,考察单因素影响情况。实验结果表明,在温度70℃、时间30min、pH为7、功率为600W条件下粗多糖的产率最高,为291.13mg/g(粗多糖/干重),远高于传统热水浸提法所得粗多糖产率(78.52mg/g,粗多糖/干重),且所得粗多糖与热水浸提法获得的粗多糖具有相似的红外光谱。说明,在一定的实验条件下,与热水浸提法相比,微波提取法不仅不会破坏多糖的结构,还有耗时短、有较高的多糖产率的优势。  相似文献   

北斗三星无源导航定位技术研究     

方兆宝  夏哲仁  赵培海  周琼华  田震华  许泽明 《海洋测绘》2007,27(2):15-17

简述北斗三星无源导航定位的原理及定位误差源。探讨用最优估计理论和方法,即卡尔曼滤波技术,消除北斗三星无源定位数据中随机误差的方法。对华南沿海北斗三星无源定位实验数据进行滤波处理,结果表明:(1)北斗三星无源定位单点定位精度在纬度方向为±58m,经度方向为±4.3m,经卡尔曼滤波后其单点定位精度在纬度方向为±43m,经度方向为±3.6m;(2)北斗三星定位误差主要分布在纬度方向;(3)通过卡尔曼滤波可使北斗三星无源定位精度提高25%。  相似文献   

利用AMSR-E对台风"泰利"的初步分析   总被引：3，自引：0，他引：3  

刘松涛  严卫  王举 《热带海洋学报》2006,25(5):26-30

基于洋面上的微波辐射传输模型,采用多元线性回归算法,建立了海洋-大气参数的反演算式,并对其进行了验证。在此基础上,根据AMSR-E的反演结果,对台风“泰利”的发生发展过程进行了初步分析。结果表明,反演算式的精度接近于网上公布的业务产品,反演结果比较符合实际情况;但是由于受到所采用物理模型的限制,反演结果对于强降水区不敏感。  相似文献   

川西盆地雾和能见度的气候特征及其对飞行的影响   总被引：1，自引：0，他引：1  

李子良  傅刚  郝丽萍 《中国海洋大学学报(自然科学版)》2007,37(2):191-196

利用川西盆地广汉机场气象台1986年1月~1995年12月共10 a地面观测资料,对广汉机场低能见度的生消时间、持续时间和能见度的年季节变化及其日变化做了统计分析,研究广汉机场全年能见度的飞行气候特征,特别是低能见度气候特征对飞行的影响。结果表明,能见度日变化特征表现为:白天早、晚时段能见度较低,午后能见度达到最高。能见度的季节变化特征表现为:冬(12,1,2月)、春季(3,4,5月)能见度较低,而夏(6,7,8月)、秋季(9,10,11月)能见度较高。冬季能见度的变化主要受辐射雾影响,夏季能见度的变化主要受降水的影响,随着降水强度的变化而变化,低能见度时间短暂。各标准低能见度逐时频率的日变化特征在各季基本相似,低能见度高频率区均出现在早晨到上午,低频率区均出现在下午。  相似文献   

Difference characteristics of sea surface temperature observed by GLI and AMSR aboard ADEOS-II     

Kohtaro Hosoda  Hiroshi Murakami  Akira Shibata  Futoki Sakaida  Hiroshi Kawamura 《Journal of Oceanography》2006,62(3):339-350

This study compares infrared and microwave measurements of sea surface temperature (SST) obtained by a single satellite. The simultaneous observation from the Global Imager (GLI: infrared) and the Advanced Microwave Scanning Radiometer (AMSR: microwave) aboard the Advanced Earth Observing Satellite-II (ADEOS-II) provided an opportunity for the intercomparison. The GLI-and AMSR-derived SSTs from April to October 2003 are analyzed with other ancillary data including surface wind speed and water vapor retrieved by AMSR and SeaWinds on ADEOS-II. We found no measurable bias (defined as GLI minus AMSR), while the standard deviation of difference is less than 1°C. In low water vapor conditions, the GLI SST has a positive bias less than 0.2°C, and in high water vapor conditions, it has a negative (positive) bias during the daytime (nighttime). The low spatial resolution of AMSR is another factor underlying the geographical distribution of the differences. The cloud detection problem in the GLI algorithm also affects the difference. The large differences in high-latitude region during the nighttime might be due to the GLI cloud-detection algorithm. AMSR SST has a negative bias during the daytime with low wind speed (less than 7 ms⁻¹), which might be related to the correction for surface wind effects in the AMSR SST algorithm.  相似文献   

高灵敏度机载L波段微波辐射计探测海表盐度     

赵凯  史久新  张汉德 《遥感学报》2008,12(2):277-283

海水盐度是研究大洋环流和全球气候变化的重要参数,L波段(1400-1427MHz)微波辐射计是进行海水盐度遥感的最有效工具.在该频段内,微波辐射亮度温度对海水盐度变化的灵敏度为0.5K/psu,而用于海洋研究的盐度分辨率为0.1-0.2psu,要求微波辐射计的灵敏度优于0.1K.高灵敏度机载L波段微波辐射计,应用数字增益波动自动补偿和温度补偿技术,保证了系统的稳定性,并采用高效的滤波技术有效地抑制了全球定位信号(GPS)对接收机的干扰,灵敏度达到0.08K.进行了多次航空和海上对比遥感试验,获得了分辨率优于0.2psu、误差精度0.42psu的测量结果.  相似文献   

非均匀月壤介质的被动微波辐射传输模拟   总被引：1，自引：1，他引：0  

孟治国  陈圣波  刘财  杜晓娟  吕航 《吉林大学学报(地球科学版)》2008,38(6)

基于非均匀月壤物理模型和辐射传输方程,模拟月壤介质中的微波辐射传输特性,探讨频率、月壤厚度等与月表亮温的关系。结果表明:在低频段,月壤微波辐射亮温的动态变化范围较大,可探测的月壤厚度大,3 GHz时的最大可探测月壤厚度达12.4 m;在高频段对应的可探测月壤厚度较小,特别是从50GHz往后的频率段内,最大可探测月壤厚度均小于2 m。不同频率的亮温-厚度变化曲线没有交叉点,且频率越高,所能探测的月壤厚度越小。根据模拟结果,建立了月壤厚度与亮温的查找表。基于查找表,利用单个波段的亮温数据即可得到月壤厚度信息。  相似文献   

被动震源进行地震勘探的可行性研究     

唐德林马文琪  胡宗正王艳伶 《中国煤炭地质》2008,20(2):46-48

为研究冲击钻机、打桩机、打夯机以及筑路机等设备工作时产生的震源,对开展工程地震勘探时的利用价值,在东庞矿2093工作面治水钻孔冲击钻进过程中进行了该项实验工作。试验采用WF-1006遥测数字地震仪及CGS-40型加速度检波器,接收排列之间方位角间隔20。,接收道数24道,道距5m,采样率1ms,记录长度2s。最近检波器距钻孔7m。利用SCHRAMM钻机产生的强大振动为被动震源,进行了250m、257m、183m、263m等不同钻井深度,以及与此相对应不同方位角（250°、250°、230°275°）的地震波接收试验。通过分析其地震记录,判定引发东庞矿矿井突水的陷落柱中心位于治水钻孔西南方向。该结论与三维地震勘探确定的陷落柱位置一致,可见通过选择合理的接收方式及参数,被动震源也能够用于地震勘探。  相似文献   

Dynamics of Mars-orbiting dust: Effects of light pressure and planetary oblateness     

A. V. Krivov  L. L. Sokolov  V. V. Dikarev 《Celestial Mechanics and Dynamical Astronomy》1995,63(3-4):313-339

This paper deals with dynamics of impact ejecta from Phobos and Deimos initially on near-circular equatorial orbits around Mars. For particles emitted in a wide size regime of 1 micron and greater, and taking into account the typical particle lifetimes to be less than 100 years, the motion is governed by two perturbing forces: solar radiation pressure and influence of Mars' oblateness. The equations of motion of particles in Lagrangian non-singular elements are deduced and solved, both analytically and numerically, for different-sized ejecta. We state that the coupled effect of both forces above is essential so that on no account can the oblateness of Mars are be neglected. The dynamics of grains prove to be quite different for the ejecta of Phobos and Deimos. For Deimos, the qualitative results are relatively simple and imply oscillations of eccentricity and long-term variations of orbital inclination, with amplitudes and periods both depending on grain size. For Phobos, the dynamics are shown to be much more complicated, and we discuss it in detail. We have found an intriguous peculiar behavior of debris near 300 µm in size. Another finding is that almost all the Phobos ejecta with radii less than 30 µm (against the values of 5 to 20 µm adopted earlier by many authors) should be rapidly lost by collisions with martian surface. The results of the paper may be the base for constructing an improved model of dust belts that presumably exist around Mars.  相似文献