共查询到20条相似文献，搜索用时 46 毫秒
1.
Jean‐Paul van Gestel Kevin D. Best Olav I. Barkved Jan H. Kommedal 《Geophysical Prospecting》2011,59(4):673-681
The frequent time‐lapse observations from the life of field seismic system across the Valhall field provide a wealth of information. The responses from the production and injection wells can be observed through time‐shift and amplitude changes. These observations can be compared to modelled synthetic seismic responses from a reservoir simulation model of the Valhall Field. The observed differences between the observations and the modelling are used to update and improve the history match of the reservoir model. The uncertainty of the resulting model is reduced and a more confident prediction of future reservoir performance is provided. A workflow is presented to convert the reservoir model to a synthetic seismic response and compare the results to the observed time‐lapse responses for any time range and area of interest. Correlation based match quality factors are calculated to quantify the visual differences. This match quality factor allows us to quantitatively compare alternative reservoir models to help identify the parameters that best match the seismic observations. Three different case studies are shown where this workflow has helped to reduce the uncertainty range associated with specific reservoir parameters. By updating various reservoir model parameters we have been able to improve the match to the observations and thereby improve the overall reservoir model predictability. The examples show positive results in a range of different reservoir modelling issues, which indicates the flexibility of this workflow and the ability to have an impact in most reservoir modelling challenges. 相似文献
2.
针对龙游地震台水位仪观测2015年3月17日出现的台阶异常现象,对比分析该台观测井2011年6-8月水淹前后的观测资料,架设临时观测仪器进行同步观测,并进行线性测试等分析,认为龙游水位仪传感器自水井被洪水淹后,因超量程而导致损坏,水位仪观测值不能真实反映井水位变化,推断此次台阶异常并非地震前兆异常。 相似文献
3.
The results of microwave observations of the solar eclipse of March 29, 2006, with the RATAN-600 radiotelescope are presented. The observations were carried out using the northeastern sector of the radiotelescope in a broad wavelength range (1.03, 1.38, 2.70, 6.20, 13.00, and 30.70 cm) in the intensity channel. The aim of the present work is to conduct a comparative analysis of the distributions of brightness temperatures in the solar atmosphere at a distance (ranging from one to two solar radii) from the center of the optical solar disk. The data for the analysis come from the RATAN-600 observations of the solar eclipse of March 29, 2006, earlier observations with the RATAN-600 radiotelescope, and calculations of brightness temperatures that were carried out using the Baumbach-Allen formula which describes the electron density in the solar corona. The differences between the distributions obtained by the above-mentioned methods are discussed. 相似文献
4.
A. R. Breen S. J. Tappin C. A. Jordan P. Thomasson P. J. Moran R. A. Fallows A. Canals P. J. S. Williams 《Annales Geophysicae》2000,18(9):995-1002
Simultaneous observations of the slow solar wind off the southeast limb of the Sun were made in May 1999 using optical measurements from the C2 and C3 LASCO coronagraphs on board the SOHO spacecraft and radio-scattering measurements from the MERLIN and EISCAT facilities. The observations show the slow solar wind accelerating outwards from 4.5 solar radii (R), reaching a final velocity of 200–300 km s-1 by 25–30 R. The acceleration profile indicated by these results is more gentle than the average profile seen in earlier LASCO observations of larger scale features, but is within the variation seen in these studies. 相似文献
5.
In the southern Northwest Territories (NWT), long time series of historical observations of climate and hydrology are scarce. Gridded datasets have been used as an alternative to instrumental observations for climate analysis in this area, but not for driving models to understand hydrological processes in the southern NWT. The suitability of temperature and precipitation from three-gridded datasets (Australian National University Spline [ANUSPLIN], ERA-Interim, and Modern-Era Retrospective Analysis for Research and Application, Version 2 [MERRA-2]) as forcings for hydrological modelling in a small subcatchment in the southern NWT are assessed. Multiple statistical techniques are used to ensure that structural and temporal attributes of the observational datasets are adequately compared. Daily minimum and maximum air temperatures in gridded datasets are more similar to observations than precipitation. The ANUSPLIN temperature time series are more statistically similar to observations, based on population statistics and temporal structure, than either of ERA-Interim or MERRA-2. The gridded datasets capture the seasonal and annual seasonal variability of precipitation but with large biases. ANUSPLIN precipitation compares better with observations than either ERA-Interim or MERRA-2 precipitation. The biases in these gridded datasets affect run-off simulations. The biases in hydrological simulations are predictable from the statistical differences between gridded datasets and observations and can be used to make informed choices about their use. 相似文献
6.
The observations in weak wind stable conditions are scarce. The present study examines the observations from the Land Surface
Processes Experiment (LASPEX) conducted at Anand, (Gujarat, India) during the year 1997–1998 to study the characteristics
of surface layer under weak wind stable conditions. The observed surface fluxes are compared with those computed using Monin-Obukhov
(M-O) similarity theory. The upper air observations and regional climatology are used to justify the persistence of weak wind
conditions at Anand. The frequency of occurrence of weak wind stable conditions is observed to be around 67%. In 86% of the
cases under weak wind conditions, bulk Richardson number (RiB) is found to be larger than 0.2. The magnitude of surface fluxes computed from M-O similarity theory is shown to be smaller
in comparison to those based on the observations in weak wind stable conditions. Surface fluxes computed using the empirical
relations for the eddy diffusivities and drag and heat exchange coefficients are found to be comparable with those based on
M-O similarity theory however these fluxes are under-predicted in comparison to the observations. The traditional M-O similarity
theory is not able to simulate the observed fluxes well in weak wind stable conditions at Anand. 相似文献
7.
The model calculations of the oceanic gravimetrical effect are compared with some recent observations. The theoretical estimates of the amplitudes and phases calculated by the ATLANTIDA3.0 program, which was developed by the authors, quite well agree with the empirical data obtained in different regions of the world. In particular, it is established that in almost 80% cases our model provides a better fit of the observations than the results calculated by the LOAD89 program of the ETERNA3.3 package developed by Wenzel. 相似文献
8.
The morphological peculiarities of the behavior of the electron density over Irkutsk (52.3° N, 104.3° E) have been investigated
by the current-median method. The observations are compared with the IRI model data at the decay phase of solar activity (2003–2006).
Systematic discrepancies between the prediction and observations are discussed. 相似文献
9.
利用1988～1999年欧洲非相干散射EISCAT（European Incoherent Scatter）雷达观测数据,对不同太阳活动周相、不同季节的极光椭圆区电离层F区电子密度进行统计分析,研究其气候学特征,并与IRI 2001模式比较.EISCAT观测到的电子密度显示出显著的太阳活动高年“冬季异常”和太阳活动低年半年变化等现象.EISCAT实测电子密度随时间和高度的平均二维分布和500 km高度以下总电子含量TEC,从总体来看与IRI 2001模式预测结果符合较好.但高年在TEC达到最大值前后,IRI 2001模式预测的电子密度高度剖面与EISCAT观测结果有显著差别：F2峰以上IRI 2001模式预测的电子密度过大,造成TEC明显高于雷达观测值.另外,在太阳活动下降相,EISCAT观测显示出明显的半年周期季节变化特征,但IRI 2001模式未能预测出此下降相季节变化. 相似文献
10.
Ocean Dynamics - In situ observations, satellite observations, and regional observations from airborne remote sensing are very useful to characterize sea state evolution and related physical... 相似文献
11.
本文选取川滇相对均匀分布的地下流体观测台点的资料,提取其中的中高频信息,然后采用幂函数衰减的方式进行中高频信息场的空间曲面拟合,研究相同物理量的多测点的短临综合信息场.川滇地下流体短临综合信息空间扫描结果表明:在川滇强震发生前短期内孕震邻近区域的短临综合信息明显出现,且大幅度起伏变化;川滇地下流体短临综合信息时间扫描结果表明:川滇强震发生前3个月内中高频信息均表现出较大幅度的增强波动变化,从而突出了震前的多台异常综合信息. 相似文献
12.
The time variability of diurnal tides was investigated by analyzing gravity observations from global superconducting gravimeter (SG) stations with running time intervals. Through least-square and Bayesian approaches, FCN resonance parameters were estimated for each data section after obtaining the tidal parameters of mainly diurnal tidal waves. The correlation of the time variation in diurnal tidal waves and FCN period was discussed. For comparison, a similar method was used to analyze VLBI observations to study the time variability of nutation terms and FCN period. The variation trend of the FCN period totally depends on the Ψ1 wave in tidal gravity and on the retrograde annual term in nutation. We observed a similar variation trend in the FCN periods obtained from different SG stations worldwide and VLBI observations. The relation between diurnal tides and LOD variations is discussed and the possible mechanisms of the decadal variation in FCN periods were discussed. 相似文献
13.
The skewness of broad Type 2-like spectra has been studied using data collected by two orthogonal CW 50-MHz radio links with co-located scattering volumes. Geometrical aspect angles of observations were about 10. One short event was considered. For this event, the electron flow direction was changing periodically (period about 9 minutes) presumably due to the passage of a magnetospheric MHD wave through the ionosphere. It was found that for the radar observations along the electrojet flow, the skewness had the same sign as the mean Doppler shift with average absolute values in between 0.5–1.0. For observations perpendicular to the electrojet flow, spectra were more symmetrical (average skewness was around 0) and the sign of the skewness was sometimes opposite to the sign of the mean Doppler shift. These observations are interpreted in terms of contribution from both the Farley-Buneman and gradient-drift instabilities to the resultant spectrum. Differences with radar observations at small aspect angles are discussed. 相似文献
14.
M. Ioualalen P. Arreaga-Vargas N. Pophet M. Chlieh K. Ilayaraja J. Ordoñez W. Renteria N. Pazmiño 《Pure and Applied Geophysics》2010,167(10):1205-1214
A numerical simulation of the 26th December, 2004 Indian Ocean tsunami of the Tamil Nadu coastal zone is presented. The simulation approach is based on a fully nonlinear Boussinesq tsunami propagation model and included an accurate computational domain and a robust coseismic source. The simulation is first confronted to available tide gauge and runup observations. The agreement between observations and the predicted wave heights allowed a reasonable validation of the simulation. As a result, a full picture of the tsunami impact is provided over the entire coastal zone Tamil Nadu. The processes responsible for coastal vulnerability are discussed. 相似文献
15.
Hindcast of oil-spill pollution during the Lebanon crisis in the Eastern Mediterranean, July-August 2006 总被引：2，自引：0，他引：2
Coppini G De Dominicis M Zodiatis G Lardner R Pinardi N Santoleri R Colella S Bignami F Hayes DR Soloviev D Georgiou G Kallos G 《Marine pollution bulletin》2011,62(1):140-153
MOON (Mediterranean Operational Oceanography Network http://www.moon-oceanforecasting.eu) provides near-real-time information on oil-spill detection (ocean color and SAR) and predictions [ocean forecasts (MFS and CYCOFOS) and oil-spill predictions (MEDSLIK)]. We employ this system to study the Lebanese oil-pollution crisis in summer 2006 and thus to assist regional and local decision makers in Europe, regionally and locally. The MEDSLIK oil-spill predictions obtained using CYCOFOS high-resolution ocean fields are compared with those obtained using lower-resolution MFS hydrodynamics, and both are validated against satellite observations. The predicted beached oil distributions along the Lebanese and Syrian coasts are compared with in situ observations.The oil-spill predictions are able to simulate the northward movement of the oil spill, with the CYCOFOS predictions being in better agreement with satellite observations. Among the free MEDSLIK parameters tested in the sensitivity experiments, the drift factor appears to be the most relevant to improve the quality of the results. 相似文献
16.
Geomagnetism and Aeronomy - The results of instrumental observations of the electric-field strength in the conditions of Moscow in 2014–2018 are presented and analyzed. The spectral... 相似文献
17.
A. Elkhalfi 《Annales Geophysicae》1999,17(4):533-546
The hydrostatic model SALSA is used to simulate a particular event observed during the Greenland Ice Margin EXperiment “GIMEX” (on July 12th, 1991). The time evolution of the large-scale flow was incorporated in the model through time dependent boundary conditions which were updated using the closest upwind sounding. A turbulent scheme for the stable boundary layer and an appropriate parametrization of the surface fluxes implemented in the same model, are used for this study. The simulation results are discussed and compared to the available observations. The computed turbulent fluxes are correctly estimated. The model predicts a mixing zone of about 1500 m high which is in good agreement with tundra site observations. Over the ice cap, the katabatic layer is correctly simulated by the model. Its height of 80–300 m is well estimated. The comparison between the simulation and observations taken at ice cap sites is reasonably valid. The ablation computed along the ice cap corresponds well to the values reconstructed of observations at sites 4 and 9. Finally, a sensibility study to a specified westward geostrophic wind (2 ms−1) shows that the consideration of this latter improves the simulated tundra wind evolution. 相似文献
18.
本文建立了利用FG5实测数据求解重力垂直梯度的数据处理模型与算法.通过对多次自由落体实验的下落距离拟合残差叠加求均值,发现下落距离观测量中存在明显的有色噪声.通过对有色噪声的建模,并以剩余残差为依据选取可靠的下落时段,解算测站点的重力垂直梯度.利用本文所提出的数据处理方法分别对FG5-214绝对重力仪在两个测站上的观测数据进行处理,以相对重力仪测量的重力垂直梯度结果为参考值,本文处理得到的重力垂直梯度结果相比于未考虑有色噪声并依据经验选取下落时段的解算方法得到了显著改善. 相似文献
19.
20.
A. V. Roldugin V. G. Vorobjev V. C. Roldugin S. A. Chernouss 《Geomagnetism and Aeronomy》2010,50(1):34-40
The results of the ground-based optical observations of sunlit auroras, performed at Lovozero and Apatity observatories on
April 10 (event 1) and April 27, 2007(event 2), are presented. The observations were performed in the (OI) 557.7 nm emission,
using a new equipment based on a Fabry-Pérot interferometer connected to a PhotonMAX CCD camera. During event 1, the observations
were performed in the Harang discontinuity region at a low magnetic disturbance. It has been indicated that an auroral arc
was located in the polar part of the eastward electrojet, and the arc position coincides with the equatorward boundary of
structured precipitation (b2e). During event 2, auroras were observed within the average statistical boundaries of the auroral
oval and the region of structured precipitation under the conditions of rather high geomagnetic activity. However, during
the period of low geomagnetic activity, discrete auroras were registered at a geomagnetic latitude of ~64° on that day, which
is 3°—4° equatorward of the structured precipitation region. Such a low latitudinal position of auroras can be explained by
the effect of a high solar wind velocity, which was ~580 km/s during the period of observations. 相似文献