共查询到20条相似文献，搜索用时 156 毫秒
1.
《中国科学:地球科学》2015,(5)
利用卫星遥感和现场观测资料,结合线性Rossby波诊断解,研究了近20年热带太平洋和印度洋暖池区海面高度的快速升高趋势.结果表明,两大洋热带区域同步的海面上升趋势通过印度尼西亚海的海洋波导通道联系在一起,其动力关联主要发生在温跃层深度,表现为热带太平洋的海面高度低频波动信号通过印度尼西亚海传至印度洋,并影响到南印度洋的东部海区,而南印度洋西部的海面变化主要受印度洋内区局地风场的调制.超前-滞后相关分析的结果表明,东南印度洋海面高度的年际和年代际变化信号分别源自太平洋赤道和近赤道海区,分别受到了太平洋赤道风应力异常和近赤道风应力旋度异常的调控,并且分别与ENSO的年际过程和PDO的年代际过程密切相关. 相似文献
2.
近海岸区域平均海面高在大地测量学、物理海洋学以及地球物理学研究中具有非常重要的意义.受各种条件的制约和限制，目前卫星测高技术主要应用于深海区域，在近海区域尤其是海岸线附近区域的应用几乎为空白.本文根据ERS-1测高卫星回波波形特征，采用五参数线性模型，由最小二乘拟合方法，对近海区域尤其是靠近海岸线附近的ERS-1测高波形数据进行波形重构.比较波形重构前、后解算平均海面高，表明波形重构技术不仅明显改善了解算近海海面高的精度，而且增加了近海测高海平面的分辨率，并使卫星测高有效观测延伸至海岸线附近.随后，本文利用波形重构后海面高数据构造了近海多年平均海平面，并对我国近海海平面特征进行了初步分析. 相似文献
3.
4.
研究了利用背向散射脉冲传播时间统计特性反演随机界面参数的问题.首先扩展了Fuks & Godin关于随机界面背向散射脉冲传播时间统计特性理论,给出了当随机界面高度-斜率统计相关情形下,最早返回的两个脉冲传播时间及其时延的概率密度函数（PDF）表达式.进而提出了一种基于背向散射脉冲传播时间统计特性的随机界面参数反演算法：采用遗传算法匹配前两个背向散射脉冲传播时间及其时延的PDF实现随机界面高度—斜率相关系数的绝对值|ρ|和无量纲参数T的反演.最后利用参数的后验概率分析反演结果的不确定性.数值模拟结果表明：该算法可有效反演随机界面的参数,参数|ρ|相对于T反演精度较高;|ρ|和T之间存在较强的参数耦合.与前人认为可忽略高度—斜率相关性（|ρ|）的观点不同：此类反演问题中应同时考虑|ρ|和T. 相似文献
5.
本文基于IRI模型、地面数字测高仪和GNSS TEC数据,提出了一种利用经验正交函数(Empirical Orthogonal Function,简称EOF)估算顶部电离层电子密度剖面的方法,并将其应用于美国Millstone Hill测高仪和GNSS数据以估算顶部电离层电子密度剖面.通过将估算的临界频率、峰值高度、400km以上电子密度分别与测高仪实测临界频率、测高仪实测峰值高度以及非相干散射雷达实测400km以上电子密度作对比以对方法的有效性进行验证.统计结果显示估算临界频率、峰值高度与测高仪实测数据基本一致,400km以上估算电子密度相较于非相干散射雷达实测的绝对误差平均值仅是测高仪推算400km以上电子密度绝对误差平均值的一半左右.所以本文提出的方法可以更加精确地估算顶部电离层电子密度. 相似文献
6.
袖珍云闪是一类区别于常规闪电放电过程的特殊放电现象,能够同时产生极强的高频和低频辐射信号,其低频辐射信号在电离层与地面之间反射后能够在电场变化波形上形成电离层反射脉冲对.电离层反射信号与原信号的时间差包含着放电三维位置和电离层高度的信息,而借助于多站闪电探测网络的同步观测就能够反演这些信息.基于这一规律,本文发展了一种对袖珍云闪实现三维定位的新方法.这种方法不仅能够对大范围内的袖珍云闪实现准确的三维定位,同时还能够反演电离层的高度,是一种潜在的研究电离层相关性质的有效手段.通过将定位结果与雷达回波比较,证明这种方法具有较高的精度.利用这种方法,计算了5489例正极性袖珍云闪和1400例负极性袖珍云闪的放电高度,发现正极性袖珍云闪主要集中在7~14 km,而负极性袖珍云闪达到了15~18 km.负极性袖珍云闪的放电高度总体上与对流层顶高度相当,其数量相比于正极性袖珍云闪明显偏少,因此很可能产生于较为罕见的极旺盛的雷暴过程中. 相似文献
7.
2001年5～7月,在冲绳岛以东海区,我们通过CTD（conductivity temperature and depth）、锚系海流剖面、PIES（pressure—recording inverted echo sounders）、卫星海面高度计和沿岸潮位仪的组合观测到一个气旋涡和一个反气旋涡．CTD断面数据显示,气旋涡和反气旋涡中心位于380／500dbar水深,对应的温度（T）和盐度（S）距平分别为-3．0,＋2．5℃和-0．20／＋0．15．从PIES数据,我们估算了气旋涡和反气旋涡经过时,相对于2000dbar深基准的动力高度（D）的时间变化为-20～30cm,500dbar深的T和S距平的变化范围约±2℃和±0．2．同时,由卫星海面高度计和潮位仪观测得到的海面高度距平变化范围约为-20至30cm,与PIES观测到的D的变化基本一致．由于两个涡经过时,PIES的压力传感器没有显示出相应的变化,反映出这两个涡具有较强的斜压特性．从卫星海面高度距平时间序列图追溯确认,这两个涡起源于北太平洋副热带逆流区附近,即20°～30°N,150°～160°E海区．它们以6cm．s^-1的平均速度向西传播了约3000km,历时约18个月,然后抵达冲绳岛以东海区． 相似文献
8.
利用曲靖非相干散射雷达2017-2018年春夏季观测数据首次分析了电离层日间150~450km电子温度的地方时与高度变化特征及其与电子密度的相关性.发现hmF2及以上的电子温度在日出日落时具有两个峰值,在11∶00-16∶00LT之间变化较小,高度越高午后上升的时间越早;从150km开始迅速增加,在约220km达到最大值,然后开始降低,在约300~350km达到最小值,最后单调上升;200km以下电子温度与电子密度成正相关(主要由热传导控制),200~450km之间存在明显的反相关(光电离过程占主导),电子-离子温度差与电子密度对数之间存在近似线性关系,电子温度逐日变化与光电离因子的变化趋势相似,这种相关性在中午与午后更明显;以上结果与其他非相干散射雷达观测和电离层模型计算结果基本一致,但也存在一些差别,需要结合更多数据深入分析. 相似文献
9.
基于频域法,利用最新的GOCE卫星重力场模型和卫星测高数据计算了稳态海面动力地形.结合海洋表层漂流浮标的观测结果,对稳态海面动力地形进行了最优空间滤波尺度分析,给出了区域、纬度带和全球稳态海面动力地形的最优空间滤波尺度因子.在此基础上,给出了全球和区域地转流.结果表明:在中高纬度和全球区域,可以分别获得空间尺度优于102km和127km的稳态海面动力地形信息.与海洋表层漂流浮标对比可知,在强流区域,采用稳态海面动力地形得到的地转流速可以解释观测浮标流速的70%;在中高纬度区域,由GOCE重力场得到的地转流略优于对应的GRACE结果;在近赤道区域,由GOCE重力场得到的地转流精度略低于对应的GRACE结果;在北大西洋和阿古拉斯强流区域,由GOCE得到的地转流场明显优于对应的GRACE结果,其精度分别提高了16%和24%. 相似文献
10.
全球定位系统多径干涉遥感技术(Global Positioning System-Interference Reflection,GPS-IR)是一种基于卫星反射信号的新遥感技术,可实现土壤湿度、雪深、海平面等方面的监测.针对卫星反射信号分离问题,本文利用小波分析对信噪比(Signal-to-Noise Ratio,SNR)中的卫星反射信号进行分离.小波基的选择直接影响到卫星反射信号分离的效果,本文通过对比低阶多项式、sym10、bior6.8、dmey和coif5这5种方法的实际消趋和反演效果来优选.经实验表明:利用coif5小波基分解6层能够有效提高卫星反射信号的分离精度和信号的分辨率,获取的相对延迟相位与土壤湿度之间的线性关系显著增强. 相似文献
11.
2022年1月8日在青海省海北州门源县发生MS6.9地震，本次地震是继2016年门源MS6.4地震后冷龙岭断裂周边发生的又一次强震。确定本次地震的破裂分布对分析该地区震害风险具有重要意义。通过收集震中及周边12个GNSS连续站点和震后加密观测的17个流动站点观测资料，获取了震中100 km范围内29个测站的GNSS静态同震形变场，并以此为约束反演了本次地震同震滑动分布。结果显示，近场GNSS观测到的最大形变量可达1.3 m。反演的最优破裂模型显示该地震主破裂区深度位于0～10 km,滑动破裂出露地表，最大滑动量为4.07 m,地震矩释放能量约1.1×1019 N·m,对应矩震级MW6.7。门源地震破裂至地表是造成该地区基础设施破坏的直接原因。 相似文献
12.
National height reference systems have conventionally been linked to the local mean sea level, observed at individual tide gauges. Due to variations in the sea surface topography, the reference levels of these systems are inconsistent, causing height datum offsets of up to ±1–2 m. For the unification of height systems, a satellite-based method is presented that utilizes global geopotential models (GGMs) derived from ESA’s satellite mission Gravity field and steady-state Ocean Circulation Explorer (GOCE). In this context, height datum offsets are estimated within a least squares adjustment by comparing the GGM information with measured GNSS/leveling data. While the GNSS/leveling data comprises the full spectral information, GOCE GGMs are restricted to long wavelengths according to the maximum degree of their spherical harmonic representation. To provide accurate height datum offsets, it is indispensable to account for the remaining signal above this maximum degree, known as the omission error of the GGM. Therefore, a combination of the GOCE information with the high-resolution Earth Gravitational Model 2008 (EGM2008) is performed. The main contribution of this paper is to analyze the benefit, when high-frequency topography-implied gravity signals are additionally used to reduce the remaining omission error of EGM2008. In terms of a spectral extension, a new method is proposed that does not rely on an assumed spectral consistency of topographic heights and implied gravity as is the case for the residual terrain modeling (RTM) technique. In the first step of this new approach, gravity forward modeling based on tesseroid mass bodies is performed according to the Rock–Water–Ice (RWI) approach. In a second step, the resulting full spectral RWI-based topographic potential values are reduced by the effect of the topographic gravity field model RWI_TOPO_2015, thus, removing the long to medium wavelengths. By using the latest GOCE GGMs, the impact of topography-implied gravity signals on the estimation of height datum offsets is analyzed in detail for representative GNSS/leveling data sets in Germany, Austria, and Brazil. Besides considerable changes in the estimated offset of up to 3 cm, the conducted analyses show that significant improvements of 30–40% can be achieved in terms of a reduced standard deviation and range of the least squares adjusted residuals. 相似文献
13.
A. Bourdillon E. Lefur C. Haldoupis Y. Le Roux J. Menard J. Delloue 《Annales Geophysicae》1997,15(7):925-934
HF radar observations of mid-latitude sporadic-E irregularities carried out with the Valensole radar in South France are compared with simultaneous ionosonde measurements underneath the irregularity zones. In a previous study of Valensole radar data, it has been shown that HF backscatter from the night-time mid-latitude E region is usually associated with largescale wave-like modulations. To obtain more information on the geophysical conditions prevailing during backscatter events, a new experiment was performed which also included a vertical ionosonde beneath the scattering region. The data to be presented here are from two periods when radar scattering appeared simultaneously with large variations in the virtual height and the Doppler velocity of F-layer reflected echoes measured with the vertical ionosonde, indicating very clearly the passage of atmospheric gravity waves (AGWs). The effect of the atmospheric waves on the sporadic-E layer is not always as marked as it is in the F region. In the first event, the passage of the AGWs is accompanied by an upward followed by a downward movement of the Es-layer. The apparent descending movement of the Es-layer from 135 to 110km in less than 10 min corresponded to a positive (downward) Doppler velocity of 35 m/s measured by the vertical ionosonde, and was accompanied by a range variation in the radar scattering region with a negative rate of about 90–110 m/s. In the second event, the Es-layer is not as strongly disturbed as in the previous one, but, nevertheless, the range variations of the scattering region can still be associated with height fluctuations of the Es-layer. 相似文献
14.
2017年8月8日的九寨沟MS7.0地震发生在岷江断裂、塔藏断裂及虎牙断裂交汇地区，地处青藏高原东北部的川甘交界地区，位于巴颜喀拉地块的东缘，地质构造复杂，对于九寨沟地震震中位置和发震断层的确定，存在不同意见.本文利用GNSS及升降轨InSAR观测，在获取九寨沟地震同震形变场的基础上，基于均匀弹性半无限位错模型，联合反演了发震断层的滑动分布模型，并计算了同震库仑应力变化.InSAR同震形变场显示，视线向最大沉降量和抬升量分别为0.21 m和0.16 m，形变场长轴为NW向，形变主要集中在断层西侧.距震中40 km和65 km的九寨和松潘两县，水平向的GNSS同震位移分别达14.31 mm和8.22 mm.联合GNSS和InSAR同震形变场反演得到的滑动分布主要集中在沿走向5~33 km，倾向2~20 km的范围内，平均滑动量为0.18 m，最大滑动量为0.91 m.发震断层长40 km，宽30 km，走向155°，倾角81°，滑动角-9.56°.同震位移场及滑移分布模型表明此次地震为一次左旋走滑为主的地震事件，地震破裂并未完全到达地表，与虎牙断裂北段的几何产状和运动学性质更为接近，结合精定位余震的分布，我们确定虎牙断裂北段为此次地震的发震断层，震中位于北纬33.25°，东经103.82°，震源深度10.86 km，矩震量为7.754×1018 Nm，相应的矩震级为MW6.5，与美国地调局和哈佛大学给出的震源机制解基本一致.同震库仑应力导致了虎牙断裂北段延长线的东北和西南两端应力增强，其中塔藏断裂的罗叉段和马磨段未来强震的危险性值得关注. 相似文献
15.
为了探明南海北部海陆过渡带的深部地壳结构,我们在香港外海域进行了一次海陆地震联洲的实验,利用固定地震台网远距离接收海上气枪信号,接收距离远达200多km,并利用此次实验的测线1剖面模拟得到了海陆过渡带的深部地壳速度结构.速度结构模型表明:研究区海陆过渡带的地壳结构非均匀性较明显,由陆至海沉积层有一个突然增厚的特点;莫霍面深度约为26～29 km,上地壳P波速度约为5.5～6.4 km/s,下地壳P波速度为6.5～6.9 km/s.在担杆列岛往海方向有一个低速破碎带,其上地壳P波速度为5.2～6.1 km/s,下地壳P波速度为6.2～6.4 km/s,结合野外地质调查的结果,推测它可能为滨海断裂带.在担杆列岛往陆方向香港和深圳之间的研究区域,莫霍面有较大起伏,可能与此处发育的海丰断裂有关. 相似文献
16.
本文利用2009年1月-2011年12月共3年的COSMIC大气掩星观测数据与SABER/TIMED探测数据开展15~60 km大气温度数据的比较分析研究,计算COSMIC与SABER/TIMED探测温度的绝对偏差(TSABER-TCOSMIC),并统计其平均温度偏差和标准偏差,分析温度偏差随高度、纬度和季节的分布特征,为COSMIC大气掩星与SABER/TIMED探测数据的应用提供更多的参考依据.结果表明:COSMIC与SABER/TIMED数据所反映的温度随高度的变化特征是一致的,数据的大体趋势吻合较好.全球范围的平均温度偏差在38 km左右接近于0 K,在38 km以上,平均温度偏差表现为负的系统性偏差,且随着高度逐渐增大,在38 km以下,平均温度偏差表现为正的系统性偏差,在23 km左右存在极大值,约为2.7 K.COSMIC与SABER/TIMED温度偏差的分布存在着随纬度和季节的变化特征,35 km以下,平均温度偏差在高纬地区和冬季较小,低纬地区和夏季较大,35 km以上,平均温度偏差在高纬地区和冬季较大,低纬地区和夏季较小.温度偏差的标准偏差在低纬地区和夏季较小,高纬地区和冬季较大.纬圈平均的温度偏差在南北半球的分布基本呈对称结构. 相似文献
17.
Conditional sampling is used herein to examine the effect of fetch, stability, and surface roughness changes on wind speeds in the coastal zone. Using data from an offshore wind farm it is shown that at a distance of 1.2–1.7 km from the coast, up to a height of 20 m above the surface, differences in wind speed distributions from onshore and offshore masts are statistically significant for flow moving offshore under all stability conditions. In contrast, differences between the distribution of wind speeds at 38 and 48 m at masts located at the coast and in the coastal zone are not significant for flow moving offshore, indicating that flow at these heights is not fully adjusted to the change in surface roughness (land to sea). These findings are in accordance with calculations of the internal boundary layer (IBL) height which indicate that the IBL would frequently be below the two upper measurement heights at 1.2–1.6 km from the coast. The analyses presented here indicate that the wind speed distribution at a potential offshore wind farm site is not solely dependent on fetch (distance from the coast) but also depends on the stability climate. 相似文献
18.
The impact of the gustiness on surface waves under storm conditions is investigated with focus on the appearance of wave groups with extreme high amplitude and wavelength in the North Sea. During many storms characterized by extremely high individual waves measured near the German coast, especially in cold air outbreaks, the moving atmospheric open cells are observed by optical and radar satellites. According to measurements, the footprint of the cell produces a local increase in the wind field at sea surface, moving as a consistent system with a propagation speed near to swell wave-traveling speed. The optical and microwave satellite data are used to connect mesoscale atmospheric turbulences and the extreme waves measured. The parameters of open cells observed are used for numerical spectral wave modeling. The North Sea with horizontal resolution of 2.5?km and with focus on the German Bight was simulated. The wind field “storm in storm,” including moving organized mesoscale eddies with increased wind speed, was generated. To take into account the rapid moving gust structure, the input wind field was updated each 5?min. The test cases idealized with one, two, and four open individual cells and, respectively, with groups of open cells, with and without preexisting sea state, as well the real storm conditions, are simulated. The model results confirm that an individual-moving open cell can cause the local significant wave height increase in order of meters within the cell area and especially in a narrow area of 1–2?km at the footprint center of a cell (the cell's diameter is 40–90?km). In a case of a traveling individual open cell with 15?m·s?1 over a sea surface with a preexisting wind sea of and swell, a local significant wave height increase of 3.5?m is produced. A group of cells for a real storm condition produces a local increase of significant wave height of more than 6?m during a short time window of 10–20?min (cell passing). The sea surface simulation from modeled wave spectra points out the appearance of wave groups including extreme individual waves with a period of about 25?s and a wavelength of more than 350?m under the cell's footprint. This corresponds well with measurement of a rogue wave group with length of about 400?m and a period of near 25?s. This has been registered at FiNO-1 research platform in the North Sea during Britta storm on November 1, 2006 at 04:00 UTC. The results can explain the appearance of rogue waves in the German Bight and can be used for ship safety and coastal protection. Presently, the considered mesoscale gustiness cannot be incorporated in present operational wave forecasting systems, since it needs an update of the wind field at spatial and temporal scales, which is still not available for such applications. However, the scenario simulations for cell structures with appropriate travel speed, observed by optical and radar satellites, can be done and applied for warning messages. 相似文献
19.
在基于GPS数据提取电离层总电子含量(TEC)的过程中,电离层薄壳高度的选择对解算电离层垂直TEC的精度有很大的影响.但由于不可能获得一个真实的从电离层D层到GPS卫星高度的电子密度剖面,关于电离层薄壳高度的选择一直是基于GPS数据解算电离层TEC方法中关注的一个问题.本文利用等离子体GCPM模型,对太阳活动高年(2002)和太阳活动低年(2008)情况下电离层有效薄壳高度的选择进行了仿真计算.结果表明,最佳的薄壳高度在2002年为560 km,而在2008年为695 km.通过对全球八个具有代表性地点的仿真计算,揭示了有效薄壳高度更复杂的变化特点.在白天,最佳薄壳的高度变化不大(500 km至750 km);但在夜晚,最佳薄壳高度变化范围很大,甚至可以超过2000 km.此外,本文还对不同卫星仰角的情况下斜向TEC转换为垂直TEC的误差进行了分析,结果表明:随着卫星仰角的增加,薄壳模型带来的转换误差基本上是单调减少的.因而,在实际应用中,尽可能地采用大仰角的卫星数据有助于提高解算的电离层垂直TEC的精度.最后,对全球不同地点的电离层TEC的仿真研究表明,在电子密度水平梯度较大的地区,应用电离层薄壳模型时会导致电子密度较高处的TEC被高估,而电子密度较低处的TEC被低估,在分析基于GPS数据提取的电离层TEC空间变化时要认识到这一点. 相似文献
20.
M. S. Solovieva A. A. Rozhnoi V. Fedun K. Schwingenschuh 《Geomagnetism and Aeronomy》2016,56(3):323-330
The analyzed amplitude and phase variations in electromagnetic VLF and LF signals at 20–45 kHz, received in Moscow, Graz (Austria), and Sheffield (UK) during the total solar eclipse of March 20, 2015, are considered. The 22 analyzed paths have lengths of 200—6100 km, are differently oriented, and cross 40–100% occultation regions. Fifteen paths crossed the region where the occultation varied from 40 to 90%. Solar eclipse effects were found only on one of these paths in the signal phase (–50°). Four long paths crossed the 90–100% occultation region, and signal amplitude and phase anomalies were detected for all four paths. Negative phase anomalies varied from–75° to–90°, and the amplitude anomalies were both positive and negative and were not larger than 5 dB. It was shown that the effective height of the ionosphere varied from 6.5 to 11 km during the eclipse. 相似文献