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Yohkoh/WBS recalibration and a comprehensive catalogue of solar flares observed by Yohkoh SXT, HXT and WBS instruments

机译:Yohkoh SXT,HXT和WBS仪器观测到的Yohkoh / WBS重新校准以及太阳耀斑的综合目录

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摘要

The flare catalogue of the Yohkoh mission is compiled and linked to this article as an electronic supplement. For showing flare characteristics over wide energy range concisely, we provide the images of Hard X-ray Telescope (HXT) and the Soft X-ray Telescope (SXT), and the spectra of Hard X-ray Spectrometer (HXS) and Gamma-Ray Spectrometer (GRS) with the Wide Band Spectrometer (WBS) time profiles. The energy versus pulse height (PH) data channels in HXS and GRS are re-calibrated by using the data of the whole mission period. Secular gain changes are recognized in HXS, and the characteristics of power-law flare spectra simultaneously observed by HXT and HXS confirms the trend. The GRS gains are different for the flare observations during the previous maximum and for the current maximum. The total of 33 gamma -ray events are observed, and for 12 of them gamma-ray flare spectra are obtained.
机译:编制了Yohkoh任务的火炬目录,并作为电子补编链接到本文。为了简明地显示宽能量范围内的耀斑特性,我们提供了硬X射线望远镜(HXT)和软X射线望远镜(SXT)的图像,以及硬X射线光谱仪(HXS)和伽马射线的光谱具有宽带光谱仪(WBS)时间配置文件的光谱仪(GRS)。通过使用整个任务期间的数据,可以重新校准HXS和GRS中的能量与脉冲高度(PH)数据通道。在HXS中可以识别出长期增益变化,并且HXT和HXS同时观察到的幂律耀斑光谱的特征证实了这一趋势。对于前一个最大值和当前最大值中的耀斑观测,GRS增益不同。总共观测到33个伽马射线事件,其中12个获得了伽马射线耀斑光谱。

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