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首页> 外文期刊>St. Petersburg Polytechnic University Journal: Physics and Mathematics >Hard X-ray time delay spectra of solar flares: BATSE spectrometer data
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Hard X-ray time delay spectra of solar flares: BATSE spectrometer data

机译：太阳能耀斑的硬X射线时间延迟光谱：Batse光谱仪数据

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摘要

A time delays of X-rays in the energy range of 20 – 200 keV registered by BATSE spectrometer during a space flight of CGRO have been considered. Pair wise correlation functions for all time series with a significant count rates were computed. Delay spectra are based via X-ray energy for different phases of flares. In the initial phase of the burst the delays increase monotonically with increasing energy. At the peak of the radiation pattern of the spectrum of different bursts is changing: from U-shaped to monotonically decreasing. On the decay phase of the count rate the delay spectra rather repeat the same of the maximum. A comparison of the delay spectra to the delays, following the models of the transport of the accelerated electrons were carried out.
机译：考虑了在CGRO空间飞行期间由Batse光谱仪注册的20-200keV能量范围内的X射线的时间延迟。计算了具有大量计数率的所有时间序列的对WIES相关功能。延迟光谱基于X射线能量，用于不同的耀斑相位。在突发的初始阶段，延迟随着能量的增加而单调地增加。在不同突发的光谱的辐射图案的峰值处变化：从U形以单调地减小。在计数阶段的衰减率上，延迟光谱相当重复相同的最大值。进行了延迟的比较，延迟，在加速电子传输的模型之后进行。

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