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Processing Radio Occultation Data by Full Spectrum Inversion Techniques: An Overview and Recent Developments

机译:通过全频谱反转技术处理无线电掩星数据:概述和最近的发展

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The Full Spectrum Inversion (FSI) method was developed in the beginning of 2002 in an effort to solve the multipath problem in radio occultation measurements. The physical ideas, which lead to the method, were that the occultation path could be considered as a synthetic aperture and the radio occultation Doppler frequency in a single path was a monotonic function of time. In star occultations, at optical wavelengths, the multipath problem is easily solved by having a lens in front of an array detector separating the beams in space. The lens is performing a spatial Fourier transform i.e., a plane wave is focused into a point displaced from the optical axis an amount given by the direction (the spatial frequency) of the plane wave. The analogy to this space processing method in time, is to have a “time lens”, which can separate multiple temporal frequencies occurring at the same time: Obviously this is what a temporal Fourier transform does. These ideas were implemented in 2001 and tested successfully on simulations of radio occultation signals, which had circular satellite orbits. However, for non-circular orbits the plain Fourier method turned out to give a not fully correct result and the work on the FSI emerged realizing that some preprocessing steps were necessary in order to eliminate the impact of non-radial orbits. This involves pre-calculation of phases, which, multiplied on the occultation signal, reduces the impact of the non-circular orbits on the resulting Fourier transform of the preprocessed signal. In 2003 the phasematching method was developed, where the impact of the non-circular orbits was totally solved, but with the cost that the processing could not be implemented with a fast Fourier transform. Both the FSI and the phasematching methods will be discussed in detail in this paper. The present development on the FSI method includes its practical implementation and making the method robust for mass processing of radio occultation signals. Filtering of signals in the FSI method is important and different filtering methods will be discussed in this paper.
机译:全谱反转(FSI)方法是在2002年初开发的,努力解决无线电常见测量中的多径问题。导致该方法的物理思想是掩护路径可以被认为是合成孔径,并且在单调的时间中的无线电掩星多普勒频率是时间的单调函数。在恒星掩星中,在光波长,通过在空间中的阵列检测器前面的镜头中具有透镜来容易解决多径问题。镜头正在执行空间傅里叶变换等。,平面波被聚焦到从光轴移位的点上由平面波的方向(空间频率)给出的量。与这种空间处理方法的比喻及时,是具有“时间镜头”,它可以同时分离多个时间频率:显然这是时间傅里叶变换的影响。这些想法是在2001年实施的,并成功地测试了对具有圆形卫星轨道的无线电掩星信号的模拟。然而,对于非圆形轨道来说,普通傅立叶方法证明了不完全正确的结果,并且FSI的工作出现了意识到需要一些预处理步骤,以消除非径向轨道的影响。这涉及阶段的预先计算,即乘以常用信号,减少了非圆形轨道对预处理信号的傅立叶变换的影响。 2003年,开发了分析方法,其中非圆形轨道的冲击完全解决,但成本与快速傅里叶变换无法实现处理。本文将详细讨论FSI和PhaseMatching方法。 FSI方法的目前的开发包括其实际实现,使方法对无线电掩星信号的批量处理稳健。在FSI方法中过滤信号是重要的,并且本文将讨论不同的过滤方法。

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