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1.
本文利用AVISO卫星高度计资料识别并追踪了北太平洋2007年—2012年的中尺度涡,并利用OSTIA的海表温度SST(Sea Surface Temperature)资料与MODIS的叶绿素a浓度(Chl-a)资料,研究了北太平洋2007年—2012年中尺度涡SST和Chl-a浓度的时空分布特征,并分析北太平洋典型中尺度涡SST与Chl-a浓度的变化特征,主要结论如下:本文共识别出992个中尺度涡,其中442个气旋涡,550个反气旋涡。中尺度涡SST时空分布特征为:气旋涡温度强度(ICE)月变化特征比反气旋涡温度强度(IAE)更强。ICE年际变化显著,IAE则不明显。温度强度较强的气旋涡和反气旋涡集中分布在黑潮延伸区。中尺度涡Chl-a浓度时空分布特征如下:气旋涡和反气旋涡Chl-a浓度月变化特征明显,且二者的变化趋势一致;年际变化则均不明显。Chl-a浓度值高的中尺度涡主要分布在高纬海域。中尺度涡SST与海洋动力参数(振幅、涡度和涡动能(EKE))的相互关系为:反气旋涡SST与振幅的相关性亦正亦负,且在空间上均匀分布。气旋涡SST与振幅的负相关系数主要分布在黑潮延伸区。正相关性强的反气旋涡多于气旋涡。反气旋涡SST与涡度的相关性亦正亦负,气旋涡SST与涡度呈负相关。反气旋涡SST与EKE的相关性亦正亦负;气旋涡的相关性为正。中尺度涡Chl-a浓度与海洋动力参数的相互关系为:反气旋涡Chl-a浓度与振幅的相关性为正,且在空间上均匀分布;气旋涡在黑潮延伸区与阿拉斯加湾呈正相关。反气旋涡和气旋涡Chl-a浓度与涡度均呈正相关。反气旋涡Chl-a浓度与EKE呈正相关;气旋涡Chl-a浓度与EKE相关性亦正亦负。 相似文献
2.
本文利用1993年—2012年AVISO卫星高度计融合数据,识别和追踪了北太平洋海域(100°E—77°W,0°N—70°N)20年的中尺度涡。统计分析了北太平洋中尺度涡的生命周期、振幅、移动速度等属性特征、空间分布和运动特征、季节、年际和年代际的变化趋势及其与ENSO的关系。结果表明:北太平洋中尺度涡的平均寿命为6.9周,平均振幅为8.44 cm,平均速度为6.4 cm/s;随着纬度的增加,反气旋涡的生命周期和振幅差异较大,气旋涡差异较小,涡旋的移动速度随纬度的增加逐渐减少。在空间分布上,日本东部的黑潮延伸区、加利福尼亚海岸和阿拉斯加湾是涡旋的高发区,其中黑潮延伸区分布最为密集;涡旋大多数向西运动,只有少数涡旋向东传播,移动过程中反气涡旋表现为向赤道方向偏移,气旋涡向极地方向偏移,且具有明显的非线性特征。在季节、年际尺度上,春季和夏季是涡旋高发的两个季节,秋季和冬季生成的涡旋相对最少,在加利福尼亚沿岸涡旋的季节差异较明显;涡旋数量的年际变化与ENSO事件具有明显的相关性,1993年—2002年厄尔尼诺年生成的涡旋较多,而拉尼娜年生成的涡旋较少,2003年—2012年则是厄尔尼诺年生成的涡旋较少,而拉尼娜年生成的涡旋较多。 相似文献
3.
中尺度涡旋具有封闭的环流结构,在海洋物质输运与能量平衡方面发挥了重要作用。观测表明海洋中涡旋并非是孤立的:气旋涡与反气旋涡倾向于相互伴随而形成稳定传播的偶极子结构。本文以1993年—2020年卫星高度计识别与追踪的中尺度涡旋数据为基础,结合涡旋的时空特征提出了偶极子涡旋的判据,建立偶极子涡旋数据集。结果表明偶极子涡旋主要分布于南北纬10°—70°纬度范围内,且平均占比约为29.53%。偶极子结构的形成对涡旋有明显的调制作用,相对于非偶极子状态,偶极子状态的涡旋振幅的增强幅度为11.09%、半径的增强幅度为7.33%、动能的增强幅度为8.58%,涡旋涡度的减小幅度为1.34%。同时,调制作用与涡旋所处的纬度和生命状态有关。在运动特征方面,偶极子状态下涡旋的传播稍有增速,变化在10%以内,而平均地转流速的最大增幅超过30%,其高值对应海洋的强流区。全球偶极子涡旋的定量分析将有助于深化对涡旋动力学的理解,为进一步剖析涡—涡相互作用机理与精细化海洋数值模拟奠定基础。 相似文献
4.
遥感影像有着丰富的纹理信息,准确地提取纹理特征对于影像的分割和分类至关重要.基于变差函数的遥感影像纹理特征提取是一种比较实用的且处于探索阶段的影像纹理分析方法.文中通过实例对提取的方法进行了研究,并通过不同变异方向纹理图像的分析比较,阐述了纹理特征准确提取应正确选取的3个因子、不同计算方向对纹理图像生成结果的影响,实验和分析还表明了变差函数法是遥感图像纹理特征提取的一种有效手段. 相似文献
5.
基于变差函数的遥感影像纹理特征提取 总被引：1，自引：0，他引：1
遥感影像有着丰富的纹理信息,准确地提取纹理特征对于影像的分割和分类至关重要。基于变差函数的遥感影像纹理特征提取是一种比较实用的且处于探索阶段的影像纹理分析方法。文中通过实例对提取的方法进行了研究,并通过不同变异方向纹理图像的分析比较,阐述了纹理特征准确提取应正确选取的3个因子、不同计算方向对纹理图像生成结果的影响,实验和分析还表明了变差函数法是遥感图像纹理特征提取的一种有效手段。 相似文献
6.
结合遥感数据与地统计学方法的海岸线超分辨率制图 总被引：1，自引：0，他引：1
使用黄河三角洲海岸Landsat卫星遥感数据,基于研究区域低分辨率6波段的海陆类型软分类结果及其变差函数,以高分辨率8波段的指示变差函数为精细尺度先验信息模型,采用数据探索性分析、协同指示克里格和序贯指示协同模拟技术,生成海陆类型发生概率模拟图像,通过等值线法提取海岸线空间分布特征。实验表明,基于地统计学方法的超分辨率制图技术在低分辨率遥感数据中融合高分辨率空间结构先验模型,可以较好表达精细尺度上的海岸线空间分布特征,同时保持原始数据的海陆类型组分信息及其空间结构特征。地统计学方法集成多尺度乃至多源空间信息的潜力通过海岸线超分辨率制图形式得到展示。 相似文献
7.
辅以纹理特征的遥感影像神经网络分类 总被引：3，自引：0，他引：3
将由变差函数提取出的纹理信息与光谱信息相结合,运用神经网络方法进行分类和地物识别,并与最大似然法的分类结果进行对比分析,结果表明该方法明显提高了遥感影像的分类精度. 相似文献
8.
变分法遥感影像人工地物自动检测 总被引：1，自引：1，他引：0
人工地物（建筑物、道路、桥梁等）检测是目标识别的一个重要组成部分。本文将人工地物检测转换为能量泛函数最优化问题。首先对遥感影像进行超像素分割,综合图像的颜色、纹理、梯度等信息,以超像素为单元计算图像的显著度信息,然后构建一个包含显著性约束、面积和边界约束、纹理约束及灰度方差约束的能量泛函数,通过变分法迭代求解能量泛函最小值,获取目标前景部分即为人工地物区域。本文以重庆和广东某地的遥感影像数据为例对算法进行验证,将其与常见的人工地物目标提取算法,如C-V模型、MRF模型,以及当下研究较为热门的深度学习算法进行对比。试验结果表明,该算法能有效地检测出遥感影像中的人工地物区域,并保证较低的误检率及漏检率。论文对该方法与深度学习方法进行了一定的分析对比。 相似文献
9.
高精度降水场是水文、气象以及环境分析的重要数据支撑,直接影响相关服务的准确性。传统降水分布模拟大多依赖站点空间维的驱动因素,而忽略了降水时序变化特征对其空间分布的影响。使用2015—2017年中国湖北省83个国家气象观测站点和28个省级观测站点近3 a月平均累积降水资料,通过相关性分析,引入站点降水时序理论变差函数模型的拱高值(C)和块金值(C0)作为影响因素,使用地理加权回归(geographically weighted regression, GWR)建立湖北省月平均降水分布模型。结果表明:（1）各站点降水的时序变差函数曲线与降水的季节性基本吻合。站点时序理论变差函数模型中,有25.3%能够在4个月内达到平稳,36.14%在6个月内达到平稳。（2）站点降水时序理论变差函数模型的C和C0与逐年12月平均累积降水在0.01水平（双侧）上显著相关,平均相关系数分别为0.745和0.526,大于地理位置和高程对降水的影响。（3）引入C和C0 有助于提升GWR模型的整体拟合优度和插值精度。对比仅使用经纬度的GWR模型和引入时序理论变差函数特征的GWR模型,3 a平均整体拟合优度从0.852提升至0.912。验证集站点插值精度评价显示,3 a绝对误差、均方根误差和平均绝对百分误差下降幅度均大于60%。因此,引入时序理论变差函数特征的时空GWR模型能够获得较高精度的降水模拟结果,更适合具有丰富历史降水资料地区的降水空间分布估算。 相似文献
10.
基于重庆CORS网的电离层VTEC插值研究 总被引：1，自引：0，他引：1
通过处理重庆CORS网的5个基准站观测数据,获得5个基准站上空电离层垂直总电子含量(VTEC)。利用其中的4个测站上空的VTEC采用克里金插值和反距离加权插值内插出另外一个测站上空VTEC。将插值结果及广义三角级数函数模型计算的电离层VTEC与实测VTEC进行比较,发现克里金插值和反距离加权插值的精度比广义三角级数函数计算的精度更高,更稳定;且克里金插值精度高于反距离加权插值。 相似文献
11.
等雨量线的绘制是济南城市防汛预警决策支持系统中最基本的功能之一。等雨量线的绘制最关键的部分为用已有站点的雨量数据进行空间插值,生成连续的雨量栅格图,再将雨量值相等的点连成等雨量线。本文用ESRI提供的ArcEngine组件实现了反距离加权插值（IDW）、样条函数插值（Spline）、克里金插值（Kriging）3种常用的插值方法,结合济南市现有的31个雨量站点的雨量数据,分别绘制出等雨量线,并比较3种插值方法的插值结果。结果表明：3种插值方法的结果都基本上反映了济南降雨的空间分布规律,而克里金插值的效果最好。 相似文献
12.
K. V. Sanil Kumar P. V. Hareesh Kumar 《Journal of the Indian Society of Remote Sensing》2005,33(1):137-146
Eddies and planetary waves are identified as one of the important factors that control the dynamics of the Arabian Sea. During
10–14 January 1990, Ignat, Paulyuchenkov (USSR ship) conducted an experiment in the central Arabian Sea and of late TOPEX/POSEIDON
satellites collected data on sea surface height (SSH) anomalies of the Arabian Sea. These data sets give an opportunity to
understand the characteristic of eddies and planetary waves in this region during winter. The geostrophic flow revealed three
anticyclonic and two cyclonic eddies of diameters ranging from 75 to more than 150 km from surface to subsurface levels. Current
speeds around different eddies were maximum at surface and varied from 9 cm/s to 25 cm/s (at the middle point between the
center and periphery). The occurrence of eddies were further investigated with the TOPEX/POSEIDON altimetry for the years
1993–97. The analysis revealed multiple eddies of diameter 100 to 550 km occur every year with maximum number of eddies during
1997 and minimum during 1995. The calculated speed varied between 8–30 cm/s around various eddies.
Longitude-Time plots showed annual Rossby waves generating at the eastern Arabian Sea and propagating westwards with a phase
speed of ~ 10 cm/s along 16° N. Further, it was observed that these waves arrived in the study area by January. In addition,
another positive anomaly of SSH was found generating at the western Arabian Sea simultaneously and extended up to the study
region by April–June. Time series of SSH at selected locations along 16°N revealed many small-scale oscillations and their
spatial variability. These oscillations were delineated using the FFT analysis. Other than the Rossby wave, the major components
at the study region were 40–60 and 26–32 day oscillations. The implications of these long period waves associated with eddies
are discussed. 相似文献
13.
海洋涡旋数量大、分布广、含能高、裹挟强,是研究物质循环、能量级联和圈层耦合的理想载体。对涡旋的全生命周期追踪观测成为21世纪以来海洋遥感领域最重要的进展之一,并引发了新一轮涡旋研究的热潮。本文从涡旋的温度异常、物质示踪、旋转流场和闭合拓扑等特征出发,简述了红外辐射计、可见光扫描仪、微波高度计、合成孔径雷达等遥感技术在涡旋观测中的机理和方法,重点阐述了卫星高度计涡旋识别与追踪算法及其在涡旋形态学、运动学和动力学中的应用。基于虚拟星座下的多参数遥感,介绍了涡旋在海洋、大气、生态等交叉学科领域的前沿应用和最新进展。指出当前涡旋遥感发展面临的亚中尺度、垂直结构、跨学科研究等3大挑战,展望了新一代遥感技术在未来海洋科学特别是涡旋海洋学研究中的应用前景。 相似文献
14.
克里格法是一种应用广泛的空间插值方法,本文研究了指示克里格法和模糊隶属度克里格法,讨论了用遗传算法对模糊隶属度克里格法进行改进的可能性及效果,并在空气污染数据插值中对3种方法的效果进行了比较。实验结果分析表明,遗传算法改进的模糊隶属度克里格插值在结果上要优于前2种方法,且具有鲁棒性较高和适应性较强等优点。 相似文献
15.
16.
Stavros A. Melachroinos Jean-Michel Lemoine Paul Tregoning Richard Biancale 《Journal of Geodesy》2009,83(10):915-923
Unmodeled sub-daily ocean S2 tide signals that alias into lower frequencies have been detected in the analysis of gravity recovery and climate experiment
(GRACE) space gravity fields of GRGS. The most significant global S2 aliased signal occurs off the northwest coast of Australia in a shallow continental shelf zone, a region with high tidal
amplitudes at a period of 161 days. The GRACE S2 aliased equivalent water height grids are convolved with Green’s functions to produce GRACE aliased tidal loading (GATL)
vertical displacements. The analysis of hourly global positioning system (GPS) vertical coordinate estimates at permanent
sites in the region confirms the presence of spectral power at the S2 frequency when the same ocean tide model (FES2004) was used. Thus, deficiencies in the FES2004 ocean tide model are detected
both directly and indirectly by the two independent space geodetic techniques. Through simulation, the admittance (ratio of
amplitude of spurious long-wavelength output signal in the GRACE time-series to amplitude of unmodeled periodic signals) of
the GRACE unmodeled S2 tidal signals, aliased to a 161-day period, is found to have a global average close to 100%, although with substantial spatial
variation. Comparing GATL with unmodeled S2 tidal sub-daily signals in the vertical GPS time-series in the region of Broome in NW Australia suggests an admittance of
110–130%. 相似文献
17.
Improving the GNSS positioning stochastic model in the presence of ionospheric scintillation 总被引：1，自引：0，他引：1
M. Aquino J. F. G. Monico A. H. Dodson H. Marques G. De Franceschi L. Alfonsi V. Romano M. Andreotti 《Journal of Geodesy》2009,83(10):953-966
Ionospheric scintillations are caused by time- varying electron density irregularities in the ionosphere, occurring more often
at equatorial and high latitudes. This paper focuses exclusively on experiments undertaken in Europe, at geographic latitudes
between ~50°N and ~80°N, where a network of GPS receivers capable of monitoring Total Electron Content and ionospheric scintillation parameters was
deployed. The widely used ionospheric scintillation indices S4 and sj{\sigma_{\varphi}} represent a practical measure of the intensity of amplitude and phase scintillation affecting GNSS receivers. However, they
do not provide sufficient information regarding the actual tracking errors that degrade GNSS receiver performance. Suitable
receiver tracking models, sensitive to ionospheric scintillation, allow the computation of the variance of the output error
of the receiver PLL (Phase Locked Loop) and DLL (Delay Locked Loop), which expresses the quality of the range measurements
used by the receiver to calculate user position. The ability of such models of incorporating phase and amplitude scintillation
effects into the variance of these tracking errors underpins our proposed method of applying relative weights to measurements
from different satellites. That gives the least squares stochastic model used for position computation a more realistic representation,
vis-a-vis the otherwise ‘equal weights’ model. For pseudorange processing, relative weights were com- puted, so that a ‘scintillation-mitigated’
solution could be performed and compared to the (non-mitigated) ‘equal weights’ solution. An improvement between 17 and 38%
in height accuracy was achieved when an epoch by epoch differential solution was computed over baselines ranging from 1 to
750 km. The method was then compared with alternative approaches that can be used to improve the least squares stochastic
model such as weighting according to satellite elevation angle and by the inverse of the square of the standard deviation
of the code/carrier divergence (sigma CCDiv). The influence of multipath effects on the proposed mitigation approach is also
discussed. With the use of high rate scintillation data in addition to the scintillation indices a carrier phase based mitigated
solution was also implemented and compared with the conventional solution. During a period of occurrence of high phase scintillation
it was observed that problems related to ambiguity resolution can be reduced by the use of the proposed mitigated solution. 相似文献
18.
Attenuation effect on seasonal basin-scale water storage changes from GRACE time-variable gravity 总被引：3，自引：0，他引：3
In order to effectively recover surface mass or geoid height changes from the gravity recovery and climate experiment (GRACE)
time-variable gravity models, spatial smoothing is required to minimize errors from noise. Spatial smoothing, such as Gaussian
smoothing, not only reduces the noise but also attenuates the real signals. Here we investigate possible amplitude attenuations
and phase changes of seasonal water storage variations in four drainage basins (Amazon, Mississippi, Ganges and Zambezi) using
an advanced global land data assimilation system. It appears that Gaussian smoothing significantly affects GRACE-estimated
basin-scale seasonal water storage changes, e.g., in the case of 800 km smoothing, annual amplitudes are reduced by about
25–40%, while annual phases are shifted by up to 10°. With these effects restored, GRACE-estimated water storage changes are
consistently larger than model estimates, indicating that the land surface model appears to underestimate terrestrial water
storage change. Our analysis based on simulation suggests that normalized attenuation effects (from Gaussian smoothing) on
seasonal water storage change are relatively insensitive to the magnitude of the true signal. This study provides a numerical
approach that can be used to restore seasonal water storage change in the basins from spatially smoothed GRACE data. 相似文献
19.
Two long time series were analysed: the C01 series of the International Earth Rotation Service and the pole series obtained
by re-analysis of the classical astronomical observations using the HIPPARCOS reference frame. The linear drift of the pole
was determined to be 3.31 ± 0.05 milliarcseconds/year towards 76.1 ± 0.80° west longitude. For the least-squares fit the a priori correlations between simultaneous pole coordinates x
p
, y
p
were taken into account, and the weighting function was calculated by estimating empirical variance components. The decadal
variations of the pole path were investigated by Fourier and wavelet analysis. Using sliding windows, the periods and amplitudes
of the Chandler wobble and annual wobble were determined. Typical periods in the variable Chandler wobble and annual wobble
parameters were obtained from wavelet analyses.
Received: 21 January 2000 / Accepted: 28 August 2000 相似文献