GOES地球同步卫星电离层电子密度剖面反演的统计验证

IF 3.4 2区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
I. Zakharenkova, I. Cherniak, Scott Gleason, Douglas Hunt, D. Freesland, A. Krimchansky, J. McCorkel, G. Ramsey, Jim Chapel
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引用次数: 0

摘要

在本文中,我们讨论了一种新的电离层电子密度剖面检索方法,该方法使用无线电掩星(RO)技术,该技术应用于两颗地球静止运行环境卫星(GOES)上的GPS接收器捕获的测量。GOES卫星的运行高度约为35800公里,主要是气象卫星,可为实时天气预报、近地环境监测和太阳观测提供连续遥感数据。GOES-16和GOES-17卫星上的GPS接收器可以跟踪在地球大气层中传播的GPS信号,尽管接收器主要设计用于导航和台站保持操作,但这些穿越地球大气层的GPS测量可以用于检索电离层电子密度剖面。这一过程带来了一系列技术挑战。GOES RO链路不同于传统的近地轨道(LEO)RO几何结构,因为接收器位于高度高于发射器的GPS星座的轨道上。此外,GOES卫星上的GPS接收器仅提供单频GPS L1观测,并且其时钟的稳定性远低于通常用于RO测量的时钟。根据以地球为中心的地球固定参考系中相对于在较低高度运行的全球定位系统星座的相对地球静止固定位置,检索到的基于地球静止轨道的RO剖面的地理分布被发现是唯一受限和可重复的,并且与基于低地球轨道的RO任务的覆盖模式显著不同。在几年的数据收集中,我们通过GOES-16和GOES-17卫星的一组具有统计学意义的GPS观测结果,证明了所提出的RO剖面技术的成功应用。这使我们能够在最高海拔1000–2000公里的情况下检索到超过10万个电离层电子密度剖面,远高于任何现有的基于LEO的RO任务。我们通过将GOES RO实验的剖面数据集与独立的参考观测(地基电离层探测和基于LEO的RO任务)进行比较,证明了基于GEO的RO测量在正确指定电离层等离子体密度的垂直分布方面具有良好的性能,以及国际参考电离层经验模型提供的模型模拟结果。经过多年的观测,对来自地球同步GOES观测的电离层F2层峰值参数(峰值密度和高度)与参考测量值之间的差异进行了统计分析。该分析揭示了GOES RO电子密度分布与F2峰和分布形状中的独立类型的测量之间的非常好的一致性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Statistical Validation of Ionospheric Electron Density Profiles Retrievals from GOES Geosynchronous Satellites
In this paper, we discuss a novel retrieval of ionospheric electron density profiles using the Radio Occultation (RO) technique applied to measurements captured by the GPS receivers on-board two Geostationary Operational Environmental Satellites (GOES). The GOES satellites operate at ~35800 km altitude and are primarily weather satellites that operationally contribute continuous remote-sensing data for real-time weather forecasting, as well as near Earth environment monitoring and Sun observations. The GPS receivers onboard GOES-16 and GOES-17 satellites can track GPS signals propagated through the Earth’s atmosphere, and although the receivers are primarily designed for navigation and station-keeping maneuvers, these GPS measurements that traverse the Earth’s atmosphere can be used to retrieve the ionospheric electron density profiles. This process poses a range of technical challenges. GOES RO links are different from the traditional low Earth orbit (LEO) RO geometry since the receiver is located in an orbit that is higher in altitude than the GPS constellation of transmitters. Additionally, the GPS receivers onboard GOES satellites provide only single frequency GPS L1 observations and have clocks much less stable than those typically used for RO measurements. The geographical distribution of the retrieved GEO-based RO profiles was found to be uniquely constrained and repeatable based on the relative geo-stationary fixed positions in the Earth Centered Earth Fixed reference frame with respect to the GPS constellation orbiting at lower altitude, and significantly different from the coverage patterns of LEO-based RO missions. We demonstrate the successful application of the proposed RO profiling technique with a statistically significant set of GPS observations from GOES-16 and GOES-17 satellites over several years of data collection. This enabled us to retrieve more than 10K ionospheric electron density profiles with a maximum altitude up to 1000–2000 km, much higher than any existing LEO-based RO mission. We demonstrate good performance of GEO-based RO measurements for properly specifying the vertical distribution of ionospheric plasma density by comparing the profiles dataset from the GOES RO experiment with independent reference observations—ground-based ionosondes and LEO-based RO missions, as well as model simulation results provided by the empirical International Reference Ionosphere model. Over multiple years of observations, statistical analysis of discrepancies between the ionospheric F2 layer peak parameters (peak density and height) derived from geosynchronous GOES observations and reference measurements was conducted. This analysis reveals a very good agreement between GOES RO electron density profiles and independent types of measurements in both the F2 peak and in the profile shape.
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来源期刊
Journal of Space Weather and Space Climate
Journal of Space Weather and Space Climate ASTRONOMY & ASTROPHYSICS-GEOCHEMISTRY & GEOPHYSICS
CiteScore
6.90
自引率
6.10%
发文量
40
审稿时长
8 weeks
期刊介绍: The Journal of Space Weather and Space Climate (SWSC) is an international multi-disciplinary and interdisciplinary peer-reviewed open access journal which publishes papers on all aspects of space weather and space climate from a broad range of scientific and technical fields including solar physics, space plasma physics, aeronomy, planetology, radio science, geophysics, biology, medicine, astronautics, aeronautics, electrical engineering, meteorology, climatology, mathematics, economy, informatics.
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