Investigation of Gas-Surface Interactions and Neutral Atmospheric Properties and Their Impact on Satellite Drag Coefficients

IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Soumyajit Dey, Phillip C. Anderson, Aaron L. Bukowski, Marcin D. Pilinski
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Abstract

Changes in the thermospheric composition and temperature influence satellite drag coefficients through functional dependencies in the closed-form solutions, and gas-surface interactions via accommodation coefficients. This study investigates drag coefficient variations for the Gravity Recovery And Climate Experiment (GRACE) and Communications/Navigation Outage Forecasting System (C/NOFS) satellites under varying atmospheric conditions and satellite orientations. The closed-form solutions of Diffuse Reflection and Incomplete Accommodation (DRIA) and Cercignani-Lampis-Lord (CLL) gas-surface interaction models have been used to calculate the drag coefficients. The momentum and energy accommodation coefficients, derived using empirical models, are used as input variables in the closed-form solutions to specify the nature of the gas-surface interactions. The results provide a realistic view of drag coefficient variations for the atmospheric changes observed for low-Earth orbit satellites. The analysis reveals that increasing the atomic oxygen mole fraction leads to significant decreases in the drag coefficients, with CLL showing greater variability than DRIA. The variability of the drag coefficients with neutral temperature demonstrates a strong dependence on satellite shapes, with GRACE drag coefficients increasing with temperature while C/NOFS drag coefficients decrease. Analysis of the C/NOFS orbits demonstrates drastic changes in the gas-surface interactions, transitioning from oxygen-dominated diffuse scattering at lower altitudes to helium-dominated quasi-specular interactions at higher altitudes. These variations persist during the September 2011 geomagnetic storm, with slightly reduced drag coefficients during storm-time conditions compared to quiet periods. The GRACE drag coefficients are highly sensitive to pitch and yaw angle variations, while the C/NOFS drag coefficients show minimal sensitivity due to its more symmetrical geometry.

Abstract Image

气体表面相互作用和中性大气特性及其对卫星阻力系数影响的研究
热层成分和温度的变化通过封闭解的函数依赖关系影响卫星阻力系数,并通过调节系数影响气体表面相互作用。本文研究了重力恢复与气候实验(GRACE)和通信/导航中断预报系统(C/NOFS)卫星在不同大气条件和卫星方向下的阻力系数变化。采用漫反射和不完全调节(DRIA)和Cercignani-Lampis-Lord (CLL)气体表面相互作用模型的封闭解计算阻力系数。利用经验模型导出的动量和能量调节系数被用作封闭形式解的输入变量,以指定气-表面相互作用的性质。这些结果为低地球轨道卫星观测到的大气变化提供了一个真实的阻力系数变化视图。分析表明,原子氧摩尔分数的增加导致阻力系数的显著降低,CLL比DRIA表现出更大的变异性。中性温度下阻力系数的变化与卫星形状密切相关,GRACE阻力系数随温度升高而增大,而C/NOFS阻力系数随温度升高而减小。对C/NOFS轨道的分析表明,气体表面相互作用发生了剧烈的变化,从低海拔以氧为主的漫射散射转变为高海拔以氦为主的准镜面相互作用。这些变化在2011年9月的地磁风暴期间持续存在,与平静期相比,风暴期间的阻力系数略有降低。GRACE阻力系数对俯仰角和偏航角变化高度敏感,而C/NOFS阻力系数由于其更对称的几何结构而表现出最小的敏感性。
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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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