一种确定太阳高能粒子起始时间及其不确定性的新方法:泊松-库苏姆自举混合法

IF 6.1 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-02-14 DOI:10.1051/0004-6361/202451280
C. Palmroos, N. Dresing, J. Gieseler, C. P. Gutiérrez, R. Vainio
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引用次数: 0

摘要

上下文。太阳高能粒子(SEP)事件是一种空间天气现象,高能带电粒子通过剧烈的喷发现象,如太阳耀斑和日冕物质抛射,从太阳释放到行星际空间。为了评估sep的起源,它们到达航天器的准确时间是至关重要的。存在几种确定观察者处SEP事件开始时间的方法,但绝大多数研究并未以系统的方式评估该开始时间的不确定性。采用一种新开发的泊松-库苏姆混合方法结合自举,我们表明,在任何特定能量范围内,与事件发生有关的不确定性往往超过测量仪器的时间分辨率,而且,它不一定与确定的开始的过去和未来对称。此外,我们还为科学界提供了一个软件工具,该软件工具可以应用所提出的方法,自动确定SEP事件发生时间及其相关不确定性,并最终允许人们轻松地进行速度色散分析。通过将Poisson-CUSUM方法与统计自举相结合应用于SEP事件观测,我们证明了该方法在合成数据和实际数据上的有效性,并将其与使用基于数据时间分辨率假设不确定性的经典方法进行的分析进行了比较。在本例中,通过速度色散分析获得的与事件相关的推断SEP路径长度和注入时间与没有正确评估不同能量下与发作时间相关的不确定性所获得的结果不同。我们还介绍了软件包PyOnset,它可以自动化该方法的许多步骤,并提供强大的数据可视化方法和分析工具。我们将代码作为开源软件发布给科学界。
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A new method for determining the onset times of solar energetic particles and their uncertainties: Poisson-CUSUM bootstrap hybrid method
Context. Solar energetic particle (SEP) events are a type of space weather phenomena in which highly energetic charged particles are released from the Sun into interplanetary space by violent and eruptive phenomena, such as solar flares and coronal mass ejections. In order to assess the origin of SEPs, an accurate timing of their arrival at spacecraft is of utmost importance. Several methods for determining the starting time of an SEP event at an observer exist, but the uncertainty of this starting time is not assessed in a systematic way by the vast majority of studies.Aims. Employing a newly developed hybrid method of Poisson-CUSUM combined with bootstrapping, we show that the uncertainty related to the onset of an event in any particular energy range is often more than the mere time resolution of the measuring apparatus, and furthermore, it is not necessarily symmetric with respect to the past and future of the determined onset. In addition, we provide a software tool to the scientific community that applies the presented method and automates the determination of SEP event onset times and their related uncertainties, and it finally allows one to easily perform a velocity dispersion analysis.Methods. By applying the Poisson-CUSUM method coupled with statistical bootstrapping to SEP event observations, we demonstrate the effectiveness of the method on synthetic and real data, and we compare them to an analysis conducted using a classical approach in which the uncertainty is assumed based on the time resolution of the data.Results. In the example case, the inferred SEP path length and injection time related to the event, acquired by the velocity dispersion analysis, differ from what is obtained without properly assessing the uncertainty related to the onset times in varying energies. We also present the software package, PyOnset, that automates many steps of the method along with providing powerful data-visualization methods and analysis tools. We release the code to the scientific community as open-source software.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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