A Comparison of Fireball Luminous Efficiency Models using Acoustic Records

Luke McFadden, Peter Brown, Denis Vida
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Abstract

The total energy of a fireball is commonly obtained from optical measurements with an assumed value for luminous efficiency. Acoustic energy measurements offer an independent means of energy estimation. Here we combine optical and acoustic methods to validate the luminous efficiency model of Borovi\v{c}ka et al. (2020). Our goal is to compare these models with acoustic measurements of meteoroid energy deposition. Employing theoretical blast scaling laws following the approach of McFadden et al. (2021), we determine explosive yields for both fireball fragmentation events and cylindrical shocks for four different bright fireballs. We model fireballs using the MetSim software (Vida et al., 2023) and find that the Borovi\v{c}ka et al. (2020) model produces agreement better than a factor of two for our three chondritic fireball case studies. The major exception is an iron meteorite-producing fireball where the luminous efficiency is an order of magnitude higher than model predictions calibrated with stony fireballs. We suggest that large disparities between optical and acoustic energies could be a signature of iron fireballs and hence useful as a discriminant of that population.
利用声学记录比较火球发光效率模型
火球的总能量通常是通过光学测量和假定的发光效率值获得的。声学能量测量提供了一种独立的能量估算方法。在这里,我们结合光学和声学方法来验证 Borovi\v{c}ka etal.(2020).我们的目标是将这些模型与流星体能量沉积的声学测量结果进行比较。我们按照麦克法登等人(2021)的方法,利用理论爆炸缩放定律,确定了四种不同亮火球的火球碎裂事件和圆柱冲击的爆炸当量。我们使用MetSim软件(Vida等人,2023年)为火球建模,发现Borovi\v{c}ka等人(2020年)的模型与我们的三个软玉体火球案例研究的一致性优于2倍。主要的例外是一个产生铁陨石的火球,它的发光效率比用石质火球标定的模型预测值高出一个数量级。我们认为,光学能量和声学能量之间的巨大差异可能是铁质火球的一个特征,因此可以用来区分铁质火球。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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