1∶500到1∶5000地形图缩编中等高线的快速生成技术     

郑志煌 《测绘与空间地理信息》2011,(3):228-230

由于1∶500与1∶5 000两种比例尺地形图中等高线的技术指标差别极大,因此要实现从1∶500到1∶5 000地形图的缩编,如何在保证质量的前提下高效地对等高线进行缩编,是一个难度很大的技术问题。文章通过探索和实验,总结出基于GeoTIN的等高线缩编技术方法,这种方法在实际生产中被证明是有效的、可靠的和具有实用性的。  相似文献   

中华绒螯蟹(Eriocheir sinensis)肠道和肝胰腺5-羟色胺(5-HT)和5-羟色胺受体2(5-HTR2)的定位研究     

杨筱珍  李彤  李萌  张佳鑫  黄坚  徐泽文  何杰  杨志刚  王春  成永旭 《海洋与湖沼》2015,46(5):1139-1145

肠道和肝胰腺是中华绒螯蟹(Eriocheir sinensis)重要的消化器官,本文运用组织学技术测量了中肠和后肠长度,并对肠道长与体长进行相关性分析。应用免疫组化技术对5-HT和5-HT受体2进行组织定位和计数。结果表明:(1)中华绒螯蟹的肠道长与体长接近,两者之间呈极显著正相关(P0.01)。后肠长度约为中肠的2倍;(2)5-HT和5-HT受体2在中肠和后肠中的组织定位和数量相似,均分布于黏膜上皮细胞间和肌层与外膜交界处,亦见于后肠的固有膜和黏膜下层与肌层交界处,在肠球外膜中也有大量分布;(3)5-HT和5-HT受体2阳性物质在肝胰腺的四种细胞的胞核中均有分布,在F细胞的胞质中也有分布。5-HT和5-HT受体2在中华绒螯蟹肠道和肝胰腺组织中的分布规律一致,表明中华绒螯蟹消化道5-HT发挥生理功能可能与5-HT受体2有关。此外,5-HT和5-HT受体2在后肠近肌细胞分布的特点可能与肠道收缩有关。后肠在中华绒螯蟹消化生理中的作用应引起重视。  相似文献   

高阶非线性完全频散性波浪数值模型及应用     

冯卫兵  邵东  王明明  张俞 《海洋工程》2015,33(1):49-57

为更精确地模拟强非线性完全频散性波浪的传播,采用长波上非线性重力表面波传播高阶数学模型,综合参考此模式已有的研究成果,建立了一个高达五阶的完全频散性非线性数值模型。应用该五阶模式对斜坡地形、潜堤地形及正弦沙链地形进行模拟计算,并与已有的实验资料进行对比,结果显示五阶模式较低阶模式模拟结果的精度上有了明显提高,模拟波形与实验结果吻合度良好,证明高阶模式更适用于高频散高非线性波浪传播的数值模拟。  相似文献   

顾及水陆差异的高分五号影像条带去除     

皮原征  储栋  管小彬  沈焕锋 《遥感学报》2020,24(4):360-367

高分五号搭载的可见光短波红外高光谱相机,能获取精细的地物光谱信息,具有十分广泛的应用前景。但高光谱卫星遥感数据往往无法避免条带噪声的干扰,进行条带去除是数据预处理中不可缺少的步骤。传统方法往往对地物的异质性与丰富的细节纹理考虑不足,导致条带不能被彻底地消除。为此,本文提出了一种顾及水陆差异的影像条带去除方法,采用水体与陆地区别统计的策略,解决条带噪声在异质区域的统计特征差异问题,并结合优化统计和一维变分滤波技术实现水陆区域参考统计特征的精确估计,最终基于矩匹配方法分别实现条带去除。实验结果表明:无论是真实实验还是模拟实验,本文提出的算法相较于传统条带去除算法,能更加稳健地去除数据条带噪声,还原地表真实辐射信息;在模拟实验中,本文算法处理结果的峰值信噪比(PSNR)达到46.58,且平均绝对误差(MAE)仅有11.56,均明显优于用于比较的3种传统算法,且算法执行效率也具备优势,能够更好地适用于高分五号大数据量的处理需求。  相似文献   

高分五号热红外传感器多通道SST反演     

崔文杰  李家国  李忠  朱利  王殿忠  张宁 《遥感学报》2020,24(7):852-866

2018-05高分五号（GF-5）卫星发射升空，其上搭载的全谱段成像仪在热红外8—13 μm谱段范围内具有4个温度反演通道（B09,B10,B11,B12），空间分辨率设计优于40 m，在国内民用传感器领域实现了由单通道向多通道、中空间分辨率向高空间分辨率的跨越式突破，使得GF-5卫星热红外数据在地表热环境遥感领域具有极其重要应用价值。本研究基于GF-5的4个热红外通道的通道响应函数，利用全球742条TIGR（Thermodynamic Initial Guess Retrieval）探空廓线数据，进行不同观测角度、水汽含量和海表发射率条件下的MODTRAN4.0（Moderate resolution atmospheric Transmittance and Radiance code4.0)辐射传输过程模拟，基于模拟结果分别对两通道、三通道和四通道劈窗算法海表温度SST（ Sea Surface Temperature）反演系数进行修订，并分析观测角度、水汽含量和海表发射率对不同通道组合的精度影响，并通过GF-5卫星实际反演的SST结果进行验证。GF-5全谱段成像仪SST反演两通道劈窗算法组合共有6种，即B09-B10、B09-B11、B09-B12、B10-B11、B10-B12、B11-B12；三通道劈窗算法组合共有4种，即B09-B10-B11、B09-B10-B12、B09-B11-B12、B10-B11-B12；四通道劈窗算法组合1种，即B09-B10-B11-B12。通过对不同通道组合形式研究发现，水汽含量对SST反演精度有较大的影响，且温度反演的精度随着水汽含量的增加而降低；其次是观测角度，SST反演精度随着观测天顶角的增大而降低；最后是发射率的影响，两通道、三通道和四通道劈窗算法SST反演精度随着发射率的变化总体在0.1 K以内变化。最后以大亚湾核电站周围海域为验证区，用GF-5热红外遥感影像进行SST的反演并做误差分析，结果表明B09-B10通道SST反演实际误差为0.57 K，反演精度较高，实际误差与理论模拟误差相差0.24 K，差异的来源主要包括辐射定标和传感器噪声等要素影响，其他通道形式反演精度有待于传感器响应稳定后进一步验证。  相似文献   

Last interglacial vegetation and climate history from the Portuguese coast          下载免费PDF全文

T. A. MINCKLEY  J. A. HAWS  M. M. BENEDETTI  S. C. BREWER  S. L. FORMAN 《第四纪科学杂志》2015,30(1):59-69

  相似文献   

条斑紫菜酵母双杂交文库的构建及PyMAPK5互作蛋白的筛选     

董道英  孔凡娜  崔正彩  孙斌 《海洋与湖沼》2019,50(6):1271-1280

为进一步研究条斑紫菜促分裂原活化激酶家族PyMAPK5的下游互作蛋白,理解其生物学功能,本研究通过酵母双杂交的方法进行其相互作用蛋白的筛选。提取不同温度和失水逆境胁迫下的RNA,利用Invitrogen体系构建条斑紫菜酵母双杂交cDNA文库,其库容为1.44×107CFU,重组率为91.8%。以pGBKT7-PyMAPK5为诱饵蛋白载体,利用共转化方法,从文库中筛选得到26个与PyMAPK5互作的候选蛋白。候选蛋白集中在光系统II相关蛋白、捕光蛋白、微管蛋白、ATP酶、GTP结合蛋白及假设蛋白等。微管蛋白、捕光蛋白、光系统II蛋白一对一验证结果为阳性,表明在酵母体内存在互作。本研究为阐明条斑紫菜PyMAPK5与其互作蛋白的关系及解析PyMAPK5下游作用机制奠定了基础。  相似文献   

The Blake Event recorded near the Eemian type locality – A diachronic onset of the Eemian in Europe     

《Quaternary Geochronology》2015

Multidisciplinary analysis including paleomagnetic, sedimentologic, sea-level change, luminescence dating and palynologic research was performed on a 25 m long orientated core taken at Rutten, close to Eemian key localities in the Netherlands. The main goal of our research was to test a possible delayed onset of temperate conditions in this region compared to Southern Europe, occurring within the Last Interglacial. The sediments revealed the presence of the paleomagnetic Blake Event in ca. 10 m of lower-deltaic floodbasin sediments that contain a pollen record covering the Eemian. The position of the Blake Event in relation to the pollen stratigraphy concurs with the earlier studied Neumark Nord 2 site. Paleomagnetic correlation to core MD95-2042 off SW Iberia indicates ca. 5 kyr diachroneity between the pollen-based onset of temperate interglacial conditions between northern and southern Europe. The onset of the Eemian in north-western and central Europe (ca. 121.0 ka) post-dates the Marine Isotope Stage 6/5e transition by ca. 10 kyr. In addition, the Rutten data provide evidence for a relatively long duration of the Blake Event of at least 8 kyr. The late onset of the temperate conditions that define the base of the Eemian, imply that NW Europe with the Eemian type area is not the most suited region to define the beginning of the Last Interglacial and Late Pleistocene for global chronostratigraphic use.  相似文献   

Remote estimation of terrestrial evapotranspiration by Landsat 5 TM and the SEBAL model in cold and high‐altitude regions: a case study of the upper reach of the Shule River Basin,China          下载免费PDF全文

Yaping Chang  Yongjian Ding  Qiudong Zhao  Shiqiang Zhang 《水文研究》2017,31(3):514-524

Evapotranspiration (ET) is an important expenditure in water and energy balances, especially on cold and high‐altitude land surfaces. Daily ET of the upper reach of the Shule River Basin was estimated using Landsat 5 TM data and the Surface Energy Balance Algorithm for Land (SEBAL) model. Based on observations made at the Suli station, the algorithms of land surface temperature and soil heat flux in SEBAL were modified. Land surface temperature was retrieved and compared with ground truth via three methods: the radiative transfer equation method, the mono‐window algorithm, and the single‐channel method. We selected the best of these methods, mono‐window algorithm, for estimating ET. The average error of daily ET estimated by the modified SEBAL model and measured by the eddy covariance system was 16.4%, with a root‐mean‐square error of 0.52 mm d^?1. The estimated ET means were 3.09, 2.48, and 1.48 mm d^?1 on June 9 (DOY 160), June 25 (DOY 176), and July 27 (DOY 208) of the year 2010, respectively. The average estimated ET on the glacier surface of all days was more than 3 mm d^?1, a measurement that is difficult to capture in‐situ and has rarely been reported. This study will improve the understanding of water balance in cold, high‐altitude regions. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

Time‐series high‐resolution spectroscopy and photometry of ε Aurigae from 2006–2013: Another brick in the wall     

K. G. Strassmeier  M. Weber  T. Granzer  L. Schanne  J. Bartus  I. Ilyin 《Astronomische Nachrichten》2014,335(9):904-934

We present continuous and time‐resolved R = 55 000 optical échelle spectroscopy of ε Aurigae from 2006–2013. Data were taken with the STELLA Echelle Spectrograph of the robotic STELLA facility at the Observatorio del Teide in Tenerife. Contemporaneous photometry with the Automatic Photoelectric Telescopes at Fairborn Observatory in Arizona is presented for the years 1996–2013. Spectroscopic observations started three years prior to the photometric eclipse and are still ongoing. A total of 474 high‐resolution échelle spectra are analyzed and made available in this paper. We identify 368 absorption lines of which 161 lines show the characteristic sharp disk lines during eclipse. Another 207 spectral lines appeared nearly unaffected by the eclipse. From spectrum synthesis, we obtained the supergiant atmospheric parameters T_eff = 7395 ± 70 K, log g ≈ 1, and [Fe/H] = +0.02 ± 0.2 with ξ_t = 9 km s^–1, ζ_RT = 13 km s^–1, and v sin i = 28 ± 3 km s^–1. The residual average line broadening expressed in km s^–1 varies with a period of 62.6 ± 0.7 d, in particular at egress and after the eclipse. Two‐dimensional line‐profile periodograms show several periods, the strongest with ≈110 d evident in optically thin lines as well as in the Balmer lines. Center‐of‐intensity weighted radial velocities of individual spectral lines also show the 110‐d period but, again, additional shorter and longer periods are evident and are different in the Balmer lines. The two main spectroscopic Hα periods, ≈ 116 d from the line core and ≈ 150 d from the center‐of‐intensity radial velocities, appear at 102 d and 139 d in the photometry. The Hβ and Johnson V I photometry on the other hand shows two well‐defined and phase‐coherent periods of 77 d and 132 d. We conclude that Hα is contaminated by changes in the circumstellar environment while the Hβ and V I photometry stems predominantly from the non radial pulsations of the F0 supergiant. We isolate the disk‐rotation profile from 61 absorption lines and found that low disk eccentricity generally relates to low disk rotational velocity (but not always) while high disk eccentricity always relates to high velocity. There is also the general trend that the disk‐absorption in spectral lines with higher excitation potential comes from disk regions with higher eccentricity and thus also with higher rotational velocity. The dependency on transition probability is more complex and shows a bi‐modal trend. The outskirts of the disk is distributed asymmetrically around the disk and appears to have been built up mostly in a tail along the orbit behind the secondary. Our data show that this tail continues to eclipse the F0 Iab primary star even two years after the end of the photometric eclipse. High‐resolution spectra were also taken of the other, bona‐fide, visual‐binary components of ε Aur (ADS 3605BCDE). Only the C‐component, a K3‐4‐giant, appears at the same distance than ε Aur but its radial velocity is in disagreement with a bound orbit. The other components are a nearby (≈ 7 pc) cool DA white dwarf, a G8 dwarf, and a B9 supergiant, and not related to ε Aur. The cool white dwarf shows strong DIB lines that suggest the existence of a debris disk around this star. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献