Statistical Distributions and Classification of X-Ray Flares According to Their Duration on the Sun

I. S. Veselovsky; A. V. Prokhorov

首页> 外文期刊>Solar system research >Statistical Distributions and Classification of X-Ray Flares According to Their Duration on the Sun

【24h】

Statistical Distributions and Classification of X-Ray Flares According to Their Duration on the Sun

机译：X射线耀斑在太阳上的持续时间的统计分布和分类

获取原文

获取原文并翻译 | 示例

掌桥外文数据库（机构版） >>

开具论文收录证明 >>

文献代查 >>

页面导航

摘要
著录项
相似文献
相关主题

摘要

The results of the statistical analysis of the GOES data related to the length of the period, during which the X-ray emission of solar flares increases, provide reliable grounds for the objective distinction of different types, sometimes referred to in the literature as typical and nontypical for bimodal classification. The events may be also partitioned into three ("impulsive", "typical", and "long duration") or more "types". These "types" should be separated from statistical fluctuations in the case of rare events. When the number of analyzed events increases, these fluctuations are gradually smoothed and become less significant, and the distribution of flares according to the duration of their growth is, on the whole, well described by the single lognormal law.

机译：GOES数据的统计分析结果与周期的长短有关，在此期间太阳耀斑的X射线发射增加，为客观区分不同类型提供了可靠的依据，在文献中有时将其称为典型值和非典型的双峰分类。事件也可以分为三种（“冲动”，“典型”和“长时间”）或更多“类型”。在罕见事件的情况下，应将这些“类型”与统计波动区分开来。当所分析事件的数量增加时，这些波动会逐渐变得平滑并且变得不那么明显，并且总体而言，耀斑根据其生长持续时间的分布可以很好地由单个对数正态定律描述。

著录项

来源
《Solar system research》 |2008年第2期|p.177-182|共6页
作者
I. S. Veselovsky; A. V. Prokhorov;
展开▼
作者单位

Skobel'tsyn Institute of Nuclear Physics, Moscow State University, 119899, Moscow, Russia;

展开▼
收录信息美国《科学引文索引》(SCI);
原文格式 PDF
正文语种 eng
中图分类天文学;
关键词

相似文献

外文文献
中文文献
专利

1. Statistical Analysis on XMM-Newton X-Ray Flares of Mrk 421: Distributions of Peak Flux and Flaring Time Duration [J] . Dahai Yan, Shenbang Yang, Pengfei Zhang, The Astrophysical journal . 2018,第2期

机译：Mrk 421的XMM-牛顿X射线耀斑的统计分析：峰通量分布和耀斑持续时间
2. New classification parameter of solar flares based on the maximum flux in soft X-rays and on duration of flare [J] . E. A. BRUEVICH Journal of astrophysics and astronomy . 2020,第6期

机译：基于软X射线的最大通量的太阳耀斑的新分类参数和闪光持续时间
3. ARE CORONAE OF MAGNETICALLY ACTIVE STARS HEATED BY FLARES? II. EXTREME ULTRAVIOLET AND X-RAY FLARE STATISTICS AND THE DIFFERENTIAL EMISSION MEASURE DISTRIBUTION [J] . MANUEL GUEDEL, MARC AUDARD, VINAY L. KASHYAP, The Astrophysical journal . 2003,第1aaParta1期

机译：耀斑是否加热了磁活跃星的冠冕？二。极紫外光和X射线耀斑统计数据以及微分排放测量值分布
4. DEM DISTRIBUTIONS FOR SHORT AND LONG DURATION FLARES AS DETERMINED FROM RESIK SOFT X-RAY SPECTRA [C] . A. Kepa, J. Sylwester, B. Sylwester, European Solar Physics Meeting . 2005

机译：从Resk软X射线光谱中确定的短期和长持续时间耀斑的DEM分布
5. Statistical study of hard X-ray solar flares. [D] . Leddon, Deborah Lynn. 2001

机译：硬X射线太阳耀斑的统计研究。
6. A Method to Estimate Sunshine Duration Using Cloud Classification Data from a Geostationary Meteorological Satellite (FY-2D) over the Heihe River Basin [O] . Bingfang Wu, Shufu Liu, Weiwei Zhu, 2014

机译：利用黑河流域对地静止气象卫星（FY-2D）的云分类数据估算日照时数的方法
7. Statistical Analysis on XMM-Newton X-Ray Flares of Mrk 421: Distributions of Peak Flux and Flaring Time Duration [O] . Dahai Yan, Shenbang Yang, Pengfei Zhang, 2018

机译：MRK 421 XMM-Newton X射线辐射统计分析：峰值通量分布和辐射时间持续时间
8. X-Ray Flare and Short-Wave Fade Duration Model. Outage Time is Directly Related to Solar Peak of X-Ray Event by Use of Event Rise Characteristics. [R] . Argo, P. E., Rothmuller, I. J., Hill, J. R. 1978

机译：X射线耀斑和短波衰落持续时间模型。通过使用事件上升特征，中断时间与X射线事件的太阳峰直接相关。

Statistical Distributions and Classification of X-Ray Flares According to Their Duration on the Sun

摘要

著录项

相似文献

相关主题

期刊订阅