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1.
This article illustrates two techniques for merging daily aerosol optical depth (AOD) measurements from satellite and ground-based data sources to achieve optimal data quality and spatial coverage. The first technique is a traditional Universal Kriging (UK) approach employed to predict AOD from multi-sensor aerosol products that are aggregated on a reference grid with AERONET as ground truth. The second technique is spatial statistical data fusion (SSDF); a method designed for massive satellite data interpolation. Traditional kriging has computational complexity O(N3), making it impractical for large datasets. Our version of UK accommodates massive data inputs by performing kriging locally, while SSDF accommodates massive data inputs by modelling their covariance structure with a low-rank linear model. In this study, we use aerosol data products from two satellite instruments: the moderate resolution imaging spectrometer and the geostationary operational environmental satellite, covering the Continental United States. 相似文献
2.
首先阐述了美国、欧洲气象卫星组织(EUMETSAT)、日本静止气象卫星的发展历史,从自旋稳定到三轴稳定,从单一载荷到多载荷并行工作,新一代的静止气象卫星的时间、空间和光谱分辨率都大幅提高,然后重点介绍了我国静止气象卫星风云二号和风云四号,相比于自旋稳定的风云二号气象卫星,风云四号卫星的功能和性能实现了跨越式的发展,接着简单介绍了俄罗斯、印度和韩国等其他国家静止气象卫星的发展状况,最后总结了不同时期各国静止气象卫星的发展特点,这对我国后续静止气象卫星的规划和研制有重要参考意义。 相似文献
3.
在NCEPGDAS中同化MSG和GOES资料 总被引：1，自引：0，他引：1
首次将MSG-2（Meteosat Second Generation-2）卫星上的旋转增强可见光及红外成像仪（Spin—ning Enhanced Visibleand Infrared Imager,SEVIRI）的观测资料同化到美国国家环境预报中心（Na—tional Centers for Environmental Prediction,NCEP）全球资料同化系统（globaldataassimilationsys—tern,GDAS）中。对当前的地球静止业务环境卫星（Geostationary Operational Environmental Satel—lite,GOES）成像仪资料的同化问题也进行了进一步探讨。利用CRTM（The Community Radiative Transfer Model）模式,对SEVIRI辐射率观测资料进行了模拟。为了对红外辐射率资料进行模拟,CRTM模式中的几个关键部分得到改进,例如：动态更新地面发射率资料以及采用了快速精确的气体吸收模块。为了改进对SEVIRI和GOES成像仪辐射率资料的模拟效果,采用了GSICS（The Global Space—Based Inter—Calibration System）标定订正。初步研究结果表明,包含对SEVIRI辐射率资料的水汽通道（6．25和7．35μm）和二氧化碳通道（13．40μm）的同化对GFS（Global Forecast System）6d预报具有显著的正影响;而对其他5个SEVIRI红外窗口通道资料的同化则减小了这种正影响。通过应用GSICS标定算法,订正了SEVIRI和GOES-12成像仪观测资料的偏差,提高了对GFS预报的影响。此外,还需作进一步研究来提高对SEVIRI红外窗口通道辐射率资料同化的有效性。 相似文献
4.
基于美国台风预报系统（Hurricane Weather Research and Forecasting,HWRF）,研究了气团订正方法对GOES-13/15静止卫星成像仪资料同化效果的改进作用,选取了2012年6月23日生成于大西洋地区的台风Debby作为研究对象,通过一组对照试验比较了气团订正前后台风路径和初始场相关物理量的差异,结果表明:气团订正能显著减小GOES-13/15静止卫星成像仪资料的系统偏差,明显提高台风路径的预报效果,气团订正使得预报的台风路径与观测路径的平均偏差和标准差降低了30%左右,提前6 h实现了台风路径的正确转向。物理机制分析表明,经过气团订正后的静止卫星资料增强了位于台风东南侧副热带高压的强度,同时增加了台风东部的温度和比湿,在引导气流和大气温、湿场的共同作用下,台风预报路径实现了正确转向。 相似文献
5.
准确的磁场模型对于辐射带粒子环境研究至关重要.本文利用美国Van Allen Probes（VAP）在2012至2018年期间测量的磁场数据和GOES15在2011至2017年期间测量的磁场数据,定量地评估了三个较新的外磁场经验模型（TS05、TA15和TA16）对外辐射带区域（3~6.6RE）磁场的描述性能.本文选择预测效率（Prediction Efficiency,PE）作为评估指标,定量分析各模型在不同空间范围（Lm值）、不同地磁活动水平（Kp）以及不同磁地方时（MLT）下的性能表现,并且计算了观测磁场与模型磁场的夹角θ,以评估模型的磁场方向预测能力.结果表明：PE随Lm值增大,随地磁扰动增强而下降;θ随Lm值增大,随地磁扰动增强而增大.在Lm=5~6.5RE范围内,PE呈现晨昏不对称性,MLT=12-21时的PE值小于MLT=0-9时的值,说明三个磁场模型可以较好地描述晨侧磁场的强度,但它们并不能很好地反映下午至昏侧磁场的大小;在地球同步轨道附近（Lm~6.6RE）,PE呈现昼夜不对称性,MLT=9-15时的PE值大于其他时区的值,说明三个磁场模型可以很好地反映昼侧磁场大小,但在夜侧可能存在较大的误差.θ在MLT=6-12时的值小于其他时区的值,呈现昼夜不对称性,说明三个磁场模型可以较好地描述昼侧磁力线的分布位型,但在夜侧存在较大的方向描述误差.在外辐射带3~6.5RE内,TA16模型与VAP磁场观测数据最为接近,PE均大于0.7,θ均小于3°;在地球同步轨道高度（6.6RE）,TS05模型与GOES15卫星磁场观测数据最为接近,PE约为0.75,θ约为7°.相关的研究结果可以为我国星载高能粒子探测器探测数据的在轨交叉定标、辐射带高能粒子动态模型研究和相关的磁层环境理论/应用研究提供地磁场模型选择方面的参考. 相似文献
6.
Markus J. Aschwanden 《Solar physics》1994,152(1):53-59
The solar 0.5–8 soft X-ray flux was monitored by the NOAA Geostationary Operational Environmental Satellites (GOES) from 1974 to the present, providing a continuous record over two solar activity cycles. Attempts have been made to determine a soft X-ray (SXR) background flux by subtracting out solar flares (using the daily lowest flux level). The SXR background flux represents the quiescent SXR flux from heated plasma in active regions, and reflects similar (intermediate-term) variability and periodicities (e.g. 155-day period) as the SXR or hard X-ray (HXR) flare rate, although it is determined in non-flaring time intervals. The SXR background flux peaks late in Solar Cycle 21 (2–3 years after the sunspot maximum), similar to the flare rate measured in SXR, HXR, or gamma rays, possibly due the increasing complexity of coronal magnetic structures in the decay phase of the solar cycle. The SXR background flux appears to be dominated by postflare emission from the dominant active regions, while the contributions from the quiet Sun are appreciable in the Solar Minimum only (A1-level). Comparisons with full-disk integrated images from YOHKOH suggest that the presence of coronal holes can decrease the quietest SXR irradiance level by an additional order of magnitude, but only in the rare case of absence of active regions.Presented at IAU Colloquium No. 143, The Sun as a Variable Star: Solar and Stellar Irradiance Variations, Boulder, CO, June 20–25, 1993 相似文献
7.
利用小波变换对GOES (Geostationary Operational Environmental Satellites)系列卫星(GOES 10/11) 1999年3月至2010年12月和风云2号系列卫星(FY 2C/2D) 2004年10月至2012年5月记录的2 MeV高能电子通量变化情况进行了相关研究,发现GOES卫星观测到的高能电子通量存在明显的13.9 d、 27.7 d、 187.0 d和342.9 d周期, FY卫星观测到的高能电子通量存在明显的13.9 d、27.7 d、222.3 d和374.0 d周期,在某些年份GOES和FY卫星均存在9 d的周期,与地磁Dst (赤道环电流指数)、 AE (极光电射流指数)指数周期高度相似.将高能电子通量和Dst、AE指数进行交叉小波分析,并利用该算法的多分辨率特点以及时域、频域局部化分析方法,将数据按不同频率进行分解,从低频系数重构图像和交叉小波谱图可以清楚看出高能电子通量和地磁指数的关系.基于FY和GOES卫星高能电子通量良好的相关性,对多卫星高能电子通量变化短周期相同、中长周期不同进一步研究,对比发现不同地磁扰动引起的GOES和FY卫星高能电子通量变化存在各向异性,小磁暴也可以对高能电子通量造成和强磁暴一样的效果,并且某些时候存在地方时一致的24 h周期.这一结果表明对地磁宁静期高能电子研究至关重要,同时对理解太阳活动,预报高能电子能谱和预警深层充电事件以及验证预测磁暴、亚暴等事件具有重要意义. 相似文献
8.
9.
《水文科学杂志》2013,58(3)
Abstract Abstract Routine estimates of daily incoming solar radiation from the GOES-8 satellite were compared to locally measured values in Florida. Longwave radiation estimates corrected using GOES-derived cloud amount and cloud top temperature products improved net radiation estimates as compared to a clear sky longwave approach. The Penman-Monteith, Turc, Hargreaves and Makkink models were applied using GOES-derived estimates of solar radiation and net radiation to predict daily evapotranspiration and were compared to evapotranspiration measured with an eddy-correlation system in an emergent wetland experimental site in north-central Florida under unstressed conditions. While the Penman-Monteith model provided the best estimates of evapotranspiration (R 2 = 0.92), the empirical Makkink method demonstrated nearly comparable agreement (R 2 = 0.90) using only the GOES solar radiation and measured temperature. The results show that it is possible to generate spatially distributed daily potential evapotranspiration estimates using GOES-derived solar radiation and net radiation with limited additional surface measurements. 相似文献
10.
The 1998 eruption of Volcan Cerro Azul, Isla Isabela, Galápagos Islands, was observed in near real-time by the Geostationary
Operational Environmental Satellite-8 (GOES-8) weather satellite. Due to the remote location of the eruption site, 3.9-μm
radiance values derived from GOES band 2 provide the best timing of the start and termination of the eruption, which occurred
on 15 Sept. and 21 Oct., respectively. Throughout the 36-day long eruption, a total of 1335 thermal infrared images were collected,
of which 851 were cloud-free and permitted the thermal anomaly to be detected. A detailed chronology including 77 separate
events was assembled from the GOES data and field observations. Numerous attributes of the eruption were observed from the
GOES data, including the sizes and dispersal of seven eruption plumes and the occurrence and timing of intra-caldera effusive
activity. The growth of a lava flow on the SE flank, the formation of smoke and volcanic haze from the flank vent, and burning
of vegetation caused by lava flows entering vegetated areas were monitored both on the ground and with the satellite data.
In most cases GOES images were processed as they were received every 30 min and were then distributed over the Internet within
minutes of reception. These data provided timely high-temporal information to field parties as well as enabled the documentation
of the eruption. The GOES observations of Cerro Azul serve as a further example of the way in which the remote sensing community
and field volcanologists can collaborate during future eruptions, and permit the temporal and spatial resolution requirements
for future satellites systems to be better defined.
Received: 27 April 1999 / Accepted: 21 February 2000 相似文献