基于参数不确定性线性随机模型的小行星与地球碰撞概率估计精度

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
V. A. Avdyushev, O. M. Syusina, V. A. Tamarov
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引用次数: 0

摘要

本文研究了基于观测资料的线性随机方法模拟的初始轨道不确定性随时间的映射所获得的小行星撞击地球概率估计的准确性。通过与非线性随机方法得到的概率进行比较,确定了估计概率的准确性。测试小行星的例子表明,如果非线性非常强,在某些观测情况下,线性方法在应用于概率评估时是不够的。线性和非线性概率估计之间的差异有时达到一个或两个数量级。此外,即使线性估计非常显著,非线性概率估计也可能为零;换句话说,在真正不存在小行星与地球相撞的风险的情况下,线性估计将错误地表明发生灾难的危险。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Accuracy of Estimation of the Probability of Asteroid Collision with the Earth Based on Linear Stochastic Modeling of Parametric Uncertainty

Accuracy of Estimation of the Probability of Asteroid Collision with the Earth Based on Linear Stochastic Modeling of Parametric Uncertainty

This paper investigates the accuracy of probabilistic estimates of asteroid impacts with the Earth obtained by mapping over time the initial orbital uncertainty modeled by linear stochastic methods based on observational material. The accuracy of the estimated probabilities is established in comparison with the probabilities obtained using nonlinear stochastic methods. The example of test asteroids shows how linear methods can be inadequate under certain observational circumstances when applied for probabilistic assessment if the nonlinearity is extremely strong. The discrepancy between linear and nonlinear probability estimates sometimes reaches one or two orders of magnitude. In addition, nonlinear probability estimates may be zero even with very significant linear estimates; in other words, in the real absence of the risk of an asteroid colliding with the Earth, linear estimates will falsely indicate the danger of a catastrophe.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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