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601.
602.
A.B. Rabiu A.O. Adewale R.B. Abdulrahim E.O. Oyeyemi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Total electron content (TEC) measured simultaneously using Global Positioning System (GPS) ionospheric monitors installed at some locations in Nigeria during the year 2011 (Rz = 55.7) was used to study the diurnal, seasonal, and annual TEC variations. The TEC exhibits daytime maximum, seasonal variation and semiannual variations. Measured TEC were compared with those predicted by the improved versions of the International Reference Ionosphere (IRI) and NeQuick models. The models followed the diurnal and seasonal variation patterns of the observed values of TEC. However, IRI model produced better estimates of TEC than NeQuick at all locations. 相似文献
603.
采用近红外漫反射光谱技术对高硅氧/酚醛预浸布的树脂含量、挥发分含量和预固化度等质量指标进行了在线测定。利用偏最小二乘法所建立的树脂含量、挥发分含量和预固化度模型的决定系数R2分别为99.20、99.14和99.11,交叉验证均方差RMSECV分别为0.298、0.144和0.124。利用外部验证集,对模型进行t-检验,在给定显著性水平0.05的情况下,近红外的测定结果和标准方法的测定结果对比,两者不存在显著性差异。该方法在预浸布生产线的应用,为其生产过程中的质量控制提供了一种有效的分析手段。 相似文献
604.
L. Perna K. Venkatesh V.G. Pillat M. Pezzopane P.R. Fagundes R.G. Ezquer M.A. Cabrera 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):295-315
Bottom side electron density profiles for two stations at the southern crest of the Equatorial Ionization Anomaly (EIA), São José dos Campos (23.1°S, 314.5°E, dip latitude 19.8°S; Brazil) and Tucumán (26.9°S, 294.6°E, dip latitude 14.0°S; Argentina), located at similar latitude and separated by only 20° in longitude, have been compared during equinoctial, winter and summer months under low (year 2008, minimum of the solar cycle 23/24) and high solar activity (years 2013–2014, maximum of the solar cycle 24) conditions. An analysis of parameters describing the bottom side part of the electron density profile, namely the peak electron density NmF2, the height hmF2 at which it is reached, the thickness parameter B0 and the shape parameter B1, is carried out. Further, a comparison of bottom side profiles and F-layer parameters with the corresponding outputs of IRI-2012 and NeQuick2 models is also reported. The variations of NmF2 at both stations reveal the absence of semi-annual anomaly for low solar activity (LSA), evidencing the anomalous activity of the last solar minimum, while those related to hmF2 show an uplift of the ionosphere for high solar activity (HSA). As expected, the EIA is particularly visible at both stations during equinox for HSA, when its strength is at maximum in the South American sector. Despite the similar latitude of the two stations upon the southern crest of the EIA, the anomaly effect is more pronounced at Tucumán than at São José dos Campos. The differences encountered between these very close stations suggest that in this sector relevant longitudinal-dependent variations could occur, with the longitudinal gradient of the Equatorial Electrojet that plays a key role to explain such differences together with the 5.8° separation in dip latitude between the two ionosondes. Furthermore at Tucumán, the daily peak value of NmF2 around 21:00 LT during equinox for HSA is in temporal coincidence with an impulsive enhancement of hmF2, showing a kind of “elastic rebound” under the action of the EIA. IRI-2012 and NeQuick2 bottom side profiles show significant deviations from ionosonde observations. In particular, both models provide a clear underestimation of the EIA strength at both stations, with more pronounced differences for Tucumán. Large discrepancies are obtained for the parameter hmF2 for HSA during daytime at São José dos Campos, where clear underestimations made by both models are observed. The shape parameter B0 is quite well described by the IRI-2012 model, with very good agreement in particular during equinox for both stations for both LSA and HSA. On the contrary, the two models show poor agreements with ionosonde data concerning the shape parameter B1. 相似文献
605.
采用全周非定常数值模拟方法,对两种畸变进口条件下的超声速压气机流场进行求解,了解动叶流场参数变化和气动性能与畸变来流条件的关系,重点分析动叶根部和顶部附近激波位置、结构和强度的变化情况,揭示动叶流场参数的动态变化规律.研究表明,随畸变区范围增加,压气机质量流量和效率下降;动叶流场参数对畸变来流的动态响应主要表现为激波位置、结构和强度的周期变化,当畸变区范围足够大时,流道在畸变区中会经历深度畸变;27.2%畸变时,畸变区内流道存在根部和顶部流动状态不一致的时刻,流场状态复杂.38.2%畸变时,畸变区内动叶叶顶和叶根区域都能达到深度畸变状态,流动损失较大且稳定性差. 相似文献
606.
607.
2009年6至7月华南地区电离层TEC扰动研究 总被引:1,自引:0,他引:1
电离层TEC(Total Electron Content)扰动与多种扰动源相关联.2009年6至7月期间存在地震和日全食的扰动源.利用广州地区GPS监测网在2009年6至7月连续监测到的TEC数据,通过采用前15天数据的滑动窗口对数据进行处理,从时间序列和空间分布两方面分析了华南地区电离层TEC扰动特征.结果显示,2009年6至7月华南地区电离层TEC扰动和该时期发生的地震以及日全食事件可能有关联;2009年7月多个地震发生引起的电离层扰动特征为,震前出现的是正异常,发震当天或震后有可能是正异常,也有可能是负异常;7月22日日全食当天TEC扰动为正异常,推测该正异常是地磁活动、地震活动及日全食综合效应的结果. 相似文献
608.
G. Meynet 《Space Science Reviews》1993,66(1-4):417-420
Let us suppose that it is possible observationally to determine the number ratio of WR to O stars in a starburst galaxy (cf. e. g. Vacca &; Conti 1992) and that one can also have some information on the way the different WR subtypes are distributed (number ratios as WN/WR, WNL/WR etc ...), the question is, what can we deduce from these values on the burst of star formation which gave birth to these WR stars? Is it possible for instance to constrain the age of the burst (i.e. the time elapsed since the beginning of the burst of star formation), its intensity (i.e. the ratio of the star formation rate during the burst to that before the burst) or the metallicity of the cloud from which the stars formed? We present here models of starbursts based on the most recent models for single stars computed by the Geneva group and show that the study of the WR population in a starburst provides very useful insights on the age of the burst and on the metallicity of the star forming zone. 相似文献
609.
Rui Tu Hongping Zhang Maorong Ge Guanwen Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
This paper proposes a method of real-time monitoring and modeling the ionospheric Total Electron Content (TEC) by Precise Point Positioning (PPP). Firstly, the ionospheric TEC and receiver’s Differential Code Biases (DCB) are estimated with the undifferenced raw observation in real-time, then the ionospheric TEC model is established based on the Single Layer Model (SLM) assumption and the recovered ionospheric TEC. In this study, phase observations with high precision are directly used instead of phase smoothed code observations. In addition, the DCB estimation is separated from the establishment of the ionospheric model which will limit the impacts of the SLM assumption impacts. The ionospheric model is established at every epoch for real time application. The method is validated with three different GNSS networks on a local, regional, and global basis. The results show that the method is feasible and effective, the real-time ionosphere and DCB results are very consistent with the IGS final products, with a bias of 1–2 TECU and 0.4 ns respectively. 相似文献
610.
为了研究含气率对液力透平内部压力的影响,以比转速为84.5的单级单吸离心泵反转作液力透平并对其内部流场进行CFD瞬态数值模拟,获得了气体在液力透平内的分布规律以及气液两相介质下透平内部流场的压力脉动变化规律。结果表明:从蜗壳进口到叶轮出口,含气率逐渐增加,含气率等于0.2时蜗壳出口、叶轮进口气体的尾迹效应明显,分布不够均匀。叶轮出口有气体聚集现象,气体体积分数越高,聚集现象越明显。进口含气率对透平蜗壳、叶轮内各点的相对压力分布影响明显,各点的相对压力随着透平进口含气率增加而降低。含气率小于0.05时其对透平内各监测点的压力脉动主频幅值影响不大,含气率大于0.05后其对液力透平内各监测点的压力脉动主频幅值有影响,含气率越高,压力脉动主频幅值越小。不同含气率下液力透平蜗壳周向、径向以及叶轮内的压力脉动主频均等于叶轮叶片的转动频率。 相似文献