高能μ子（> 230 GeV）的气压效应
Barometric Effect of High-Energy Muons (> 230 GeV)
摘要：
根据Baksan地下闪烁望远镜数据，获得了十年（2003-2012年）六个粒子登记天顶角间隔的气压系数。得到的气压系数比理论值高出一个数量级。然而，这些结果与其他作者的一些论文中关于高能μ子气压效应的数据是一致的。随着μ子阈值能量的增加，测量气压系数的绝对值有明显的增加。
英文摘要：
According to the Baksan underground scintillation telescope data the barometric coefficients for six intervals of zenith angles of particle registration were obtained for ten years (2003-2012). The obtained barometric coefficients exceed an order of magnitude the theoretical values. Nevertheless, these results are in good agreement with the data obtained for the barometric effect of high-energy muons in a number papers of other authors. And there is a noticeable increase of the absolute values of the measured barometric coefficients with increase of the threshold energy of muons.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
