Inferring Fireball Velocity Profiles and Characteristic Parameters of Meteoroids From Incomplete Data Sets

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Eloy Peña-Asensio, Maria Gritsevich
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引用次数: 0

Abstract

Extracting additional information from old or incomplete fireball data sets remains a challenge. To address missing point-by-point observations, we introduce a method for estimating atmospheric flight parameters of meteoroids using metaheuristic optimization techniques. Using a fireball catalog from the European Fireball Network (EN), we reconstruct velocity profiles, meteoroid bulk densities, mass loss rates, and ablation and ballistic coefficients, based on the initial and terminal points' height, velocity, and mass with the purely dynamical α $\alpha $ - β $\beta $ model. Additionally, the method's performance is compared to the Meteorite Observation and Recovery Project (MORP) derived fits, confirming the robustness of the computed parameters for objects with asteroidal compositions. Our findings show that α $\alpha $ - β $\beta $ model yields parameters consistent with the photometric and dynamic mass estimates in the EN catalog for P E ${P}_{E}$ type I events. However, in the implementation proposed here, α $\alpha $ - β $\beta $ model encounters limitations in accurately representing the final deceleration of more fragile high-velocity meteoroids. This is likely due to challenges in representing complex fragmentation processes by fitting only two points, even when initial and terminal residuals are minimal. The retrieved α $\alpha $ - β $\beta $ distribution differs from the one derived from MORP data, likely due to the imposed mass constraints, which strongly influence the results, especially the bulk density. The results suggest that P E ${P}_{E}$ constraints reduce fitting accuracy (from 90% to 44%), while flexibility and freedom from assumptions improve α $\alpha $ - β $\beta $ performance. The method yields 26% of the events compatible with the catalog P E ${P}_{E}$ classification. Our approach is well-suited for interpreting historical or sparse data sets.

从不完全数据集推断流星体的火球速度剖面和特征参数
从旧的或不完整的火球数据集中提取额外的信息仍然是一个挑战。为了解决缺少逐点观测的问题,我们介绍了一种使用元启发式优化技术估计流星体大气飞行参数的方法。利用欧洲火球网络(EN)的火球目录,我们根据初始点和终点的高度、速度、质量损失率、烧蚀和弹道系数,重建了速度剖面、流星体体积密度、质量损失率和弹道系数。质量与纯动力学α $\alpha $ - β $\beta $模型。此外,将该方法的性能与陨石观测与回收项目(MORP)的衍生拟合进行了比较,证实了计算参数对小行星组成物体的鲁棒性。我们的研究结果表明,α $\alpha $ - β $\beta $模型得到的参数与EN目录中pe的光度和动态质量估计值一致${P}_{E}$ I类事件。然而,在本文提出的实现中,α $\alpha $ - β $\beta $模型在准确表示更脆弱的高速流星体的最终减速时遇到了限制。这可能是由于仅通过拟合两点来表示复杂破碎过程的挑战,即使初始和终端残差很小。反演得到的α $\alpha $ - β $\beta $分布与MORP数据的分布不同,这可能是由于施加的质量约束,这强烈影响了结果,尤其是体积密度。结果表明,P E ${P}_{E}$约束降低了拟合精度(从90% to 44%), while flexibility and freedom from assumptions improve α $\alpha $ - β $\beta $ performance. The method yields 26% of the events compatible with the catalog P E ${P}_{E}$ classification. Our approach is well-suited for interpreting historical or sparse data sets.
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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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