使用Ørsted GPS测量电离层层析成像-初步结果

A. Escudero ∗ , A.C. Schlesier , A. Rius , A. Flores , F. Rubek , G.B. Larsen , S. Syndergaard , P. Høeg
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引用次数: 13

摘要

来自丹麦Ørsted卫星上的Turbo-Rogue GPS接收器的数据用于推导卫星对卫星的总电子含量(TEC)。我们提出了利用TEC Ørsted数据从电离层层析获得电子密度场的初步结果。TEC基于单频测量,因为只有L1信号质量好。C/A伪量程(C1)和L1相位用于获得TEC测量。基于阿贝尔变换,推导了单个掩星的电子密度分布图,并与层析解进行了比较。在阿贝尔变换中,球面对称的假设限制了剖面的精度,并经常导致偏差。我们选择沿轨道平面观测的掩星以最小化球面不对称效应。层析网格也被限制在靠近轨道平面的狭窄环面。TEC的计算是基于6小时(3.6个轨道)周期的数据。本次研究选取了1999年12月5日和1999年2月12日这两天。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ionospheric tomography using Ørsted GPS measurements - preliminary results

Data from the Turbo-Rogue GPS receiver onboard the Danish Ørsted Satellite are used to derive satellite-to-satellite Total Electron Content (TEC). We present preliminary results obtaining Electronic Density fields from ionospheric tomography using TEC Ørsted data. TEC is based on single frequency measurements, since only the L1 signal is of good quality. The C/A pseudo range (C1) and the L1 phase are used to obtain the TEC measurement. Electron density profiles from individual occultations are derived, based on the Abel transform, and compared with the tomographical solution. The assumption of spherical symmetry in the Abel transform limits the accuracy of the profiles and often results in a bias. We select occultations observed along the orbital plane to minimize the spherical assymetry effects. The tomographic grid is also confined to a narrow torus close to the orbital plane. The TEC calculations are based on data from 6 hour (3.6 orbits) periods. Two days have been selected for this study, December 5, 1999 and February 12, 1999.

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