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The frequency distribution for several characteristics of a solar flare obeys a power law only above a certain threshold, below which there is an apparent loss of small scale events presumably caused by limited instrumental sensitivity and th:e corresponding event selection bias. It is also possible that this deviation in the power law can have a physical origin in the source. We propose two fitting models incorpo- rating a power law distribution with a low count rate cutoff plus a noise component for the frequency distribution of the hard X-ray peak count rate of all solar flare sam- ples obtained with HXRBS/SMM and BATSE/CGRO observations. Our new fitting method produces the same power-law index as previously developed methods, a low cutoff of the power-law function and its corresponding noise level, which is consistent with measurements of the actual noise level of the hard X-ray count rate. We found that the fitted low cutoff appears to be related to the noise level, i.e., flares are only recognized when their peak count rate is 3or greater than noise. Therefore, the fitted low cutoff, which is smaller than the aforementioned threshold, might be attributed to selection bias, and probably not to the actual count rate cutoff in flares at smaller scales. Whether or not the actual low cutoff physically exists needs to be checked by future observations with increased sensitivities. 相似文献
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根据低能伽玛射线在沉积地层中的吸收理论,推导出了低能伽玛伽玛计数率与沉积地层岩性参数之产是的关系式,并通过实例定性地分析了这种关系的存在。 相似文献
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本文提出用特征 X射线的发射和吸收来测定薄层或表面涂层的厚度。从理论上解决了最佳能量的选择问题 ,使薄层厚度测定的检出下限大幅度优化。并通过实践证明了方法的可靠性和实用性 相似文献
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SF-1型岩石声发射测试仪是岩石力学实验研究的一种非常有用的测试仪器。它可以用来监测岩石或岩石样品在外力作用下,发生变化过程中由微破裂所产生的声发射现象。它不仅可以研究微破裂与应力、变形、波速、时间等的变化规律,而且还可以进一步研究微破裂与主破裂(大破裂)的关系。所以它在岩石或岩体的变形破坏实验研究中具有重要的意义。多年来,在进行岩石力学研究中一直缺少适用的声发射仪,从而影响了这方面工作的开展。为了当前 相似文献
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