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首页> 外文期刊>Journal of Space Weather and Space Climate >Accuracy assessment of the quiet-time ionospheric F2 peak parameters as derived from COSMIC-2 multi-GNSS radio occultation measurements
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Accuracy assessment of the quiet-time ionospheric F2 peak parameters as derived from COSMIC-2 multi-GNSS radio occultation measurements

机译:从COSMIC-2多GNSS无线电掩星测量源自宇宙-2多GNSS无线电掩星测量的安静时间电离层F2峰值参数的准确性评估

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The Constellation Observing System for Meteorology, Ionosphere, and Climate 2 (COSMIC-2) mission was launched into a low-inclination (24°) orbit on June 25, 2019. Six satellites, each with an advanced Tri-GNSS Radio-Occultation Receiver System (TGRS), provide a global and uniform data coverage of the equatorial region with several thousand electron density profiles daily. The COSMIC-2 electron density profiles, and specifically the derived ionospheric F2 peak parameters, are properly validated in this study with reliable “truth” observations. For this purpose, we used manually scaled ionograms from 29 ground-based ionosondes located globally at low and middle latitudes. For this validation campaign, we considered only geomagnetically quiet conditions in order to establish benchmark level of the new mission’s ionospheric observation quality and to evaluate the operational capability of the COSMIC-2 Radio Occultation (RO) payload at the background of normal day-to-day variability of the ionosphere. For reliable colocations between two independent techniques, we selected only COSMIC-2 RO profiles whose F2 peak point coordinates were within 5° of the closest ionosonde. Our comparison of the ionospheric F2 peak height (hmF2) derived from COSMIC-2 RO and ground-based ionosonde measurements showed a very good agreement, with a mean of ~5 and ~2?km at low and middle latitudes, respectively, while RMS error was of ~23 and ~14?km, respectively. That range corresponds to a deviation of only 6–9% from the reference, ionosonde observations. Examination of representative collocation events with multiple (2–5) simultaneous RO tracks near the same ionosonde with different RO geometry, multi-satellite and multi-GNSS combination give us observational evidence that COSMIC-2 RO-based EDPs derived from GPS and GLONAS links show good self-consistency in terms of the ionospheric F2 peak values and electron density profile shape. We can conclude that COSMIC-2 provides high quality data for specification the ionospheric electron density at the F2 peak region.
机译:气象,电离层和气候2(COSMIC-2)特派团的星座观测系统于2019年6月25日推出了轨道下降(24°)轨道。六个卫星,每个卫星都有先进的三GNSS无线电扫描器系统(TGRS),每天提供具有几千个电子密度型材的赤道区域的全局和均匀数据覆盖。宇宙-2电子密度型材,特别是衍生的电离层F2峰值参数,在本研究中正确验证了可靠的“真相”观察。为此目的,我们在低于和中纬度地区的29个地面的INOOSONDES中使用了手动缩放离子图。对于这种验证活动,我们只考虑了地磁安静的条件,以建立新的任务的电离层观察质量的基准水平,并评估宇宙-2无线电园(RO)有效载荷的正常日背景的运行能力 - 电离层的日变异性。对于两个独立技术之间的可靠分层,我们只选择了宇宙-2 RO曲线,其F2峰值坐标位于最近的IONOSONDE的5°内。我们对来自宇宙-2 RO的电离层F2峰值高度(HMF2)的比较和基于基于地基的Ionosonde测量结果表现出非常良好的一致性,平均值分别在低和中纬度的〜5〜2 km处,同时rms误差分别为约23〜14 km。该范围对应于来自参考,Ionosonde观察的6-9%的偏差。与多个有代表性的搭配事件的考试(2-5)同时RO轨道不同RO几何形状,多星,多GNSS组合相同的电离层探测仪附近给我们的观测证据表明,基于RO-COSMIC-2 EDPS从GPS和GLONAS导出链接在电离层F2峰值和电子密度轮廓形状方面显示出良好的自我稠度。我们可以得出结论,COSMIC-2提供了高质量的数据,用于规范F2峰值区的电离层电子密度。

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