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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Correlations Between the Thermosphere’s Semiannual Density Variations and Infrared Emissions Measured With the SABER Instrument
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Correlations Between the Thermosphere’s Semiannual Density Variations and Infrared Emissions Measured With the SABER Instrument

机译:之间的相关性热电离层的半年密度变化和红外排放用军刀仪器测量

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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, https://doi.org/10.1029/2009JA014102, 2015b, https://doi.org/10.1002/2015JA021047) 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:本文提出测量振幅和计时的结合、年度和半年的变化thermospheric中立密度,比较这些密度红外测量的变化排放二氧化碳和一氧化氮热大气层。从测量获得的大气拖挑战Minisatellite经历有效载荷、重力恢复与气候实验一、重力场和海洋环流的探险家,和三个群卫星,而光排放测量的探测使用宽带发射辐射线测定大气(剑)仪器热大气层电离层中间层能量学和动力学卫星。这些数据跨16年的时间。数据库包含全球平均密度来自大约5000的轨道对象(挥拳相向,2009,https://doi.org/10.1029/2009JA014102, 2015 b,https://doi.org/10.1002/2015JA021047)是用于校准这些密度数据。与NRLMSISE-00模型被用来进行比较获得多少密度的测量随着时间的推移,由于这些季节性变化变化。振动有明显的变化振幅和时间。使用光学排放作为一种实用性的监控工具,军刀数据是适合的测量变化。只使用过滤二氧化碳排放有很好的相关性测量振荡。也预测了一个简单的傅里叶系列,与最初的预期。然而,测量光预计热大气层排放在未来的理解和有一个角色吗半年变化的预测。

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