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Improving capabilities of broadband differential satellite navigation systems via radio occultation technology

机译:通过无线电掩星技术提高宽带差分卫星导航系统的能力

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摘要

The existent satellite system for radio occultation monitoring the Earth's neutral atmosphere and ionosphere (COSMIC) provides data to consumers in the regions with limited possibilities of constructing dense measurement networks (e.g., in the World Ocean area). A forthcoming increase of LEO small spacecrafts and the deployment of new satellite radio navigation systems will result in a pronounced increase in the efficiency of radio occultation method and its space resolution. As a result, the Space-Based Augmentation Systems (SBAS) broadband differential system will become global, or the quality of corrections delivered to single-frequency consumers of individual systems, e.g., the Augmentation and Monitoring System, will be improved. Therefore, the methods for processing and analyzing obtained radio occultation data should be improved. A simple method to reconstruct the electron density profile at radio occultation points, based on the total electron content measurement on the satellite-satellite path and the IRI-type ionospheric model has been proposed. The method needs initial information, it does not require refraction measurements, and it is free of the assumption that the ionosphere is spherically stratified in the occultation region. Verification of the proposed method based on data for 121 radio occultation cases across Europe in May 2013 demonstrated good agreement with the vertical sounding data.
机译:现有的用于监视地球的中性大气和电离层的无线电掩星的卫星系统(COSMIC)可为区域内的消费者提供数据,而这些地区构建密集的测量网络的可能性有限(例如,在世界海洋地区)。 LEO小型航天器的即将增加和新卫星无线电导航系统的部署将导致无线电掩星方法的效率及其空间分辨率得到显着提高。结果,天基增强系统(SBAS)宽带差分系统将成为全球性的,或者将改善向增强和监测系统等单个系统的单频用户提供的校正质量。因此,应该改进用于处理和分析获得的无线电掩星数据的方法。提出了一种基于卫星卫星路径上的总电子含量测量和IRI型电离层模型重建无线电掩星点电子密度分布的简单方法。该方法需要初始信息,不需要折射测量,并且无需假设电离层在掩星区域呈球形分层。根据2013年5月在欧洲范围内121例无线电隐匿病例的数据对提议的方法进行的验证表明,该方法与垂直探测数据具有很好的一致性。

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