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Ionospheric conductances derived from satellite measurements of auroral UV and X-ray emissions, and ground-based electromagnetic data: a comparison

机译:从卫星对极光UV和X射线发射的测量以及地面电磁数据得出的电离层电导:比较

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Global instantaneous conductance maps can be derived from remotesensing of UV and X-ray emissions by the UVI and PIXIE camerason board the Polar satellite. Another technique called the 1-D method ofcharacteristics provides mesoscale instantaneous conductanceprofiles from the MIRACLE ground-based network in NorthernScandinavia, using electric field measurements from the STAREcoherent scatter radar and ground magnetometer data from the IMAGEnetwork. The method based on UVI and PIXIE data gives conductancemaps with a resolution of ~800km in space and ~4.5minin time, while the 1-D method of characteristicsestablishes conductances every 20s and with a spatialresolution of ~50km. In this study, we examine three periodswith substorm activity in 1998 to investigate whether the twotechniques converge when the results from the 1-D method ofcharacteristics are averaged over the spatial and temporalresolution of the UVI/PIXIE data.

In general, we find that the calculated conductance sets do notcorrelate. However, a fairly good agreement may be reached whenthe ionosphere is in a state that does not exhibit strong localturbulence. By defining a certain tolerance level of turbulence,we show that 14 of the 15 calculated conductance pairs duringrelatively uniform ionospheric conditions differ less than ±30%.The same is true for only 4 of the 9 data points derivedwhen the ionosphere is in a highly turbulent state. A correlationcoefficient between the two conductance sets of 0.27 is derivedwhen all the measurements are included. By removing the datapoints from time periods when too much ionospheric turbulenceoccurs, the correlation coefficient raises to 0.57. Consideringthe two very different techniques used in this study to derive theconductances, with different assumptions, limitations and scalesizes, our results indicate that simple averaging of mesoscaleresults allows a continuous transition to large-scale results.Therefore, it is possible to use a combined approach to studyionospheric events with satellite optical and ground-basedelectrodynamic data of different spatial and temporal resolutions.We must be careful, though, when using these two techniques duringdisturbed conditions. The two methods will only give results thatsystematically converge when relatively uniform conditions exist.

机译:可以通过Polar卫星上的UVI和PIXIE摄像头对UV和X射线发射进行遥感来获得全局瞬时电导图。另一种称为一维特征方法的技术使用来自STARE相干散射雷达的电场测量和来自IMAGE网络的地面磁力计数据,从NorthernScandinavia的MIRACLE地面网络提供中尺度瞬时电导曲线。基于UVI和PIXIE数据的方法给出的电导图在空间上的分辨力约为800km,在时间上约为4.5min,而一维特征法则每20s建立电导,空间分辨率约为50km。在这项研究中,我们研究了1998年的三个具有亚暴活动的时期,以研究将一维特征方法的结果在UVI / PIXIE数据的时空分辨率上求平均值时,两种技术是否会收敛。

通常,我们发现计算出的电导率集不相关。但是,当电离层处于不显示强局部湍流的状态时,可能会达成相当好的协议。通过定义一定的湍流容限水平,我们表明在相对均匀的电离层条件下计算出的15个电导对中的14个相差小于±30%。当电离层处于高度湍流时,得出的9个数据点中只有4个是正确的州。当包括所有测量值时,得出两个电导集之间的相关系数为0.27。通过从发生电离层湍流过多的时间段中删除数据点,相关系数提高到0.57。考虑到本研究中使用两种截然不同的技术来推导电导,具有不同的假设,局限性和规模大小,我们的结果表明,对中尺度结果进行简单平均可以连续转换为大规模结果,因此可以使用组合方法使用具有不同时空分辨率的卫星光学和地面电动力数据来研究电离层事件。但是,在扰动条件下使用这两种技术时,我们必须小心。当存在相对一致的条件时,这两种方法只会给出系统收敛的结果。

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