PMO OpenIR  > PMO中文期刊
耀斑软X射线流量的统计性质
张平; 刘四明
2015
Source Publication天文学报
Issue1Pages:35-43
Abstract为了更定量地研究太阳耀斑软X射线辐射的统计性质,发展了一套对于给定峰值流量区间的耀斑的自动识别程序,并用它分析了从1980年到2013年GOES(Geostationary Operational Environmental Satellite)在两个软X射线波段上对太阳耀斑的观测.研究发现耀斑软X射线流量在峰值附近变化的统计特征和耀斑流量峰值的绝对大小无关:平均而言耀斑流量的上升时间约是下降时间的一半,而且高能量通道的上升和下降时间比相应的低能量通道时间要短,但是这些时间还是会随着耀斑流量变化幅度的增加而增加.
Language中文
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/14932
CollectionPMO中文期刊
Recommended Citation
GB/T 7714
张平,刘四明. 耀斑软X射线流量的统计性质[J]. 天文学报,2015(1):35-43.
APA 张平,&刘四明.(2015).耀斑软X射线流量的统计性质.天文学报(1),35-43.
MLA 张平,et al."耀斑软X射线流量的统计性质".天文学报 .1(2015):35-43.
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