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Beacon Satellite Symposium: Session 5B - June 30th 2016: Radio Occultation Techniques and Measurements

机译:信标卫星研讨会:分会场5B-2016年6月30日:无线电掩星技术和测量

摘要

During the Beacon Satellite Symposium, held in Trieste, Italy, between June 26 and July 1 2016, the JRC chaired the session 5B: Radio Occultation Techniques and Measurements. The corresponding abstract of the session is provided as follows:Since the mid-1960s, the GNSS based radio occultation technique has been used to study the structure and properties of the atmospheres of not only Earth but also other planets, such as Venus, Mars, some other outer planets, and many of their moons. By measuring the phase delay of radio waves from GNSS satellites as they are occulted by the Earth’s atmosphere, the vertical density profiles of the bending angles of radio wave trajectories can be estimated using measurements onboard LEO satellites. The success of the GPS/MET mission in 1995 inspired a number of follow‐on missions that include radio occultation experiment, including the CHAMP, GRACE, SAC-C, COSMIC, Metop-A/B, C/NOFS, and upcoming COSMIC-2 satellites. The combined profiles from these different LEO satellites provide excellent opportunities to explore the dynamics and structure of the ionosphere, especially in the regions that have been devoid of ground-based instruments, allowing for investigation of the longitudinal variability of the ionospheric density structure. This session seeks contributions that advance the application of RO technique for space weather studies. In addition, we welcome presentations exploring innovative methodologies that address the current problem on RO inversion technique at the equatorial region where ionospheric irregularity, such as sporadic E and spread F, present and degrade the linear combination technique that affect the quality of density profile extracted in the region.The session was organized among Endawoke Yizengaw (Institute for Scientific Research, Boston College), Jann-Yenq Liu (National Space Organization –NSPO- Chief Scientist), and Angela Aragon-Angel (Joint Research Centre). The session consisted of both oral and poster presentation parts.This document presents the process of the session preparation within the Beacon Satellite Symposium organization. Moreover, the abstracts of the different contributions accepted to the session are also included for completeness.
机译:在2016年6月26日至7月1日在意大利的里雅斯特举行的信标卫星研讨会上,JRC主持了会议5B:无线电掩星技术和测量。会议的摘要如下:自1960年代中期以来,基于GNSS的无线电掩星技术被用于研究地球以及其他行星(如金星,火星,其他一些外行星,以及它们的许多卫星。通过测量GNSS卫星在地球大气层中所掩藏的无线电波的相位延迟,可以使用LEO卫星上的测量来估算无线电波轨迹弯曲角的垂直密度分布。 1995年GPS / MET任务的成功激发了许多后续任务,其中包括无线电掩星实验,包括CHAMP,GRACE,SAC-C,COSMIC,Metop-A / B,C / NOFS和即将推出的COSMIC- 2颗卫星。来自这些不同LEO卫星的组合廓线为探索电离层的动力学和结构提供了极好的机会,尤其是在没有地面仪器的地区,从而可以研究电离层密度结构的纵向变化。本届会议寻求有助于推进反渗透技术在空间天气研究中的应用的贡献。此外,我们欢迎您进行演讲,探讨创新的方法论,以解决电离层不规则性(例如零星E和散布F)存在并降低影响密度分布质量的线性组合技术的赤道地区赤道区域反渗透技术的当前问题。会议由波士顿大学科学研究所的Endawoke Yizengaw,国家航天组织(NSPO)首席科学家Jann-Yenq Liu和联合研究中心的Angela Aragon-Angel组织。会议包括口头报告和海报展示两部分。本文件介绍了信标卫星专题讨论会组织内的会议筹备过程。此外,为了完整起见,还包括了会议接受的不同贡献的摘要。

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    ARAGON ANGEL MARIA ANGELES;

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  • 年度 2016
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  • 正文语种 ENG
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