Debris falling forecast method for spacecraft disintegrating separation

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Dun Li, Zhi-Hui Li, Yue-Long He, Jing-Jiang Chu, Yu Jiang
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引用次数: 0

Abstract

Large spacecraft fall out of orbit and re-enter the atmosphere at the end of their lifetime, and they can break up into small debris upon re-entry. The spacecraft debris generated by the disintegration may lead to high risk when the surviving debris reaches the ground. One way to reduce the damage risk of spacecraft is to simulate the spacecraft disintegration process and accurately predict the falling area. Aerodynamics seriously affects the reentering process, especially in the continuous flow regime. Aerodynamic force and heat are the main factors leading to debris disintegration. High dynamic pressure leads to sharp changes in attitude and complex trajectories during debris fall. A numerical method based on an unstructured Cartesian grid was developed to simulate the disintegrating separation problem by coupling the Navier-Stokes equation and the six-degree-of-freedom trajectory equation. A method combining the numerical method for dynamic processes with numerical simulation based on a static aerodynamic/dynamic characteristic database was developed for forecasting the falling area. Spacecraft disintegrating separation from 60 km was simulated using the method, and the multibody aerodynamic interference and the separation trajectory were predicted. The falling process was forecast by a numerical simulation method based on the static aerodynamic database/dynamic characteristic database when the debris went out of the influence domain. This method has good forecasting efficiency while considering the aerodynamic interference, making it a valuable method for forecasting disintegrating separation and falling debris.

航天器解体分离碎片下落预测方法
大型航天器在其寿命结束时脱离轨道并重新进入大气层,它们在重新进入大气层时会分解成小碎片。解体产生的航天器碎片在幸存的碎片到达地面时可能会导致高风险。降低航天器损坏风险的一种方法是模拟航天器解体过程并准确预测坠落面积。空气动力学严重影响再入过程,尤其是在连续流动状态下。空气动力和热量是导致碎片崩解的主要因素。在碎片坠落过程中,高动态压力会导致姿态的急剧变化和复杂的轨迹。通过耦合Navier-Stokes方程和六自由度轨迹方程,提出了一种基于非结构笛卡尔网格的数值方法来模拟崩解分离问题。基于静态气动/动态特性数据库,提出了一种将动态过程的数值方法与数值模拟相结合的方法来预测坠落面积。利用该方法模拟了航天器在60km外的解体分离,并预测了多体气动干扰和分离轨迹。采用基于静态气动数据库/动态特性数据库的数值模拟方法,对碎片脱离影响域时的坠落过程进行了预测。该方法在考虑空气动力学干扰的情况下具有良好的预测效率,是预测崩解分离和碎片下落的一种有价值的方法。
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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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