用地震数据追踪空间碎片的重新进入和解体动态
Benjamin Fernando1, Constantinos Charalambous2
1Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA.
概括
在重新进入时跟踪空间碎片是很困难的,但一种新的地震逆转方法可以准确地确定轨迹和碎片化. 这提高了空间局势意识和碎片危险减轻的预测.
科学领域:
- 太空科学 太空科学
- 地质物理学 地质物理学
- 航空航天工程 航空航天工程
背景情况:
- 增加的轨道拥堵增加了不受控制的太空碎片重新进入的风险.
- 目前的方法难以准确预测碎片沉位置,因为在大气燃烧期间的跟踪限制.
研究的目的:
- 开发和验证一种用于分析大气中的太空碎片重返地球的动态的新方法.
- 为了提高碎片轨迹,大小和碎片化模式的预测准确度.
主要方法:
- 展示了一个最小梯度适合的地震逆转方法.
- 将该方法应用于2024年深-15再入事件的开源数据.
主要成果:
- 成功地发现了大气中的碎片轨迹,速度,高度,下降角度,大小和碎片.
- 从最初预测的轨道显著向南的重新进入位置得出.
- 观测到级联式的,多重的碎片化模式,为解体动态提供了见解.
结论:
- 地震逆转方法提供了一种快速可靠的方法来分析太空碎片的重返.
- 通过这种改进的追踪能力,可以提高空间局势意识和减轻碎片危险.
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