EUV Irradiance Inputs to Thermospheric Density Models: Open Issues and Path Forward
EUV Irradiance Inputs to Thermospheric Density Models: Open Issues and Path Forward
复制标题
EUV 辐照度输入热层密度模型：悬而未决的问题和前进的道路
DOI：
--
复制
发表时间：
2018
期刊：
影响因子：
--
通讯作者：
S. Bruinsma
中科院分区：
文献类型：
--
作者：
A. Vourlidas;S. Bruinsma
NASA“与星同行”研究所关于“近地轨道（LEO）航天器大气阻力的临近预报”的目标之一，是研究是否以及如何通过提高太阳强迫输入（即极紫外线（EUV）辐照度信息）的质量来提高大气阻力模型的准确性。在这篇重点综述中，我们研究了EUV测量和代理的现状和问题，讨论了最近有希望的发展，并提出了一些方法来提高下一个太阳周期EUV测量的可靠性、可用性和预测精度。
One of the objectives of the NASA Living With a Star Institute on “Nowcasting of Atmospheric Drag for low Earth orbit (LEO) Spacecraft” was to investigate whether and how to increase the accuracy of atmospheric drag models by improving the quality of the solar forcing inputs, namely, extreme ultraviolet (EUV) irradiance information. In this focused review, we examine the status of and issues with EUV measurements and proxies, discuss recent promising developments, and suggest a number of ways to improve the reliability, availability, and forecast accuracy of EUV measurements in the next solar cycle.