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Correlations Between the Thermospheres Semiannual Density Variations and Infrared Emissions Measured With the SABER Instrument

机译:用SABRE仪器测量的热圈半年度密度变化与红外发射之间的相关性

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摘要

This paper presents measurements of the amplitudes and timings of the combined, annual, and semiannual variations of thermospheric neutral density, and a comparison of these density variations with measurements of the infrared emissions from carbon dioxide and nitric oxide in the thermosphere. The density values were obtained from measurements of the atmospheric drag experienced by the Challenging Minisatellite Payload, Gravity Recovery and Climate Experiment A, Gravity field and Ocean Circulation Explorer, and three Swarm satellites, while the optical emissions were measured with the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics satellite. These data span a time period of 16 years. A database containing global average densities that were derived from the orbits of about 5,000 objects (Emmert, 2009, , 2015b, ) was employed for calibrating these density data. A comparison with the NRLMSISE‐00 model was used to derive measurements of how much the density changes over time due to these seasonal variations. It is found that the seasonal density oscillations have significant variations in amplitude and timing. In order to test the practicality of using optical emissions as a monitoring tool, the SABER data were fit to the measured variations. Even the most simple fit that used only filtered carbon dioxide emissions had good correlations with the measured oscillations. However, the density oscillations were also well predicted by a simple Fourier series, contrary to original expectations. Nevertheless, measurements of the optical emissions from the thermosphere are expected to have a role in future understanding and prediction of the semiannual variations.
机译:本文介绍了热球中性密度的组合,年度和半年度变化的幅度和时间的测量,并将这些密度变化与热球中二氧化碳和一氧化氮的红外辐射的测量结果进行了比较。密度值是通过对具有挑战性的微型卫星有效载荷,重力恢复和气候实验A,重力场和海洋环流探测器以及三颗Swarm卫星所经历的大气阻力进行测量而获得的,而光发射是通过使用大气探测法测量的热球电离层中层能量与动力学卫星上的宽带辐射辐射(SABER)仪器。这些数据的时间跨度为16年。包含从大约5,000个物体的轨道中导出的全球平均密度的数据库(Emmert,2009年,2015b)用于校准这些密度数据。通过与NRLMSISE-00模型进行比较,得出了由于这些季节性变化导致密度随时间变化多少的度量。发现季节性密度振荡在幅度和时间上有很大的变化。为了测试使用光发射作为监视工具的实用性,将SABRE数据与所测得的变化进行拟合。即使是仅使用过滤的二氧化碳排放量的最简单拟合也与测得的振荡具有良好的相关性。但是,与最初的预期相反,通过简单的傅立叶级数也可以很好地预测密度振荡。尽管如此,热球光学发射的测量有望在未来对半年变化的理解和预测中发挥作用。

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