英语翻译The shape of the dip can be used for the energy calibration of the detectors.Shifting the energies by a factor λ for each detector in the energy interval of the dip((1-40) x 10^18eV) one can determing the minimum X^2 and from it deduce t

英语翻译The shape of the dip can be used for the energy calibration of the detectors.Shifting the energies by a factor λ for each detector in the energy interval of the dip((1-40) x 10^18eV) one can determing the minimum X^2 and from it deduce t
英语翻译
The shape of the dip can be used for the energy calibration of the detectors.Shifting the energies by a factor λ for each detector in the energy interval of the dip((1-40) x 10^18eV) one can determing the minimum X^2 and from it deduce the value of λ that best fits the data.This procedure leads to λ1=0.9,λ2=1.2 and λ3=0.75 for AGASA,HiRes and Yakutsk detector ,respectively.It is worth noticing that the required correction factor is less than unity for ground arrays and exceeds unity for fluorescence experiments.It is impressive that after this shift (calibration by the dip) the spectra of these three detectors agree very well (see Fig.3).The result shown in Fig .3 have already been presented by some of us at different conferences starting from 2004 (see e.g.[36]).Recently AGASA collaboration [37] has reduced the energies by about 10% as we predicted.

英语翻译The shape of the dip can be used for the energy calibration of the detectors.Shifting the energies by a factor λ for each detector in the energy interval of the dip((1-40) x 10^18eV) one can determing the minimum X^2 and from it deduce t
形状下探可以用于能量校正的探测器.将能量由一个因素对每种探测器的λ能量区间的下降((1-40)x 10 ^ 18eV)可以决定最低x ^ 2和它的价值,演绎λ最适合的数据.这个过程导致λ1 = 0.9,λ2 = 120和λ3 = 0.75为AGASA,雇佣和Yakutsk检测器,分别是. 值得注意到所需的修正系数小于团结统一为地面阵列和超过对荧光的实验.它是令人印象深刻的,这种转变(校正后,由倾角)的光谱这三个探测器(见图很一致,结果显示在图3已由我们中的一些人在不同的会议,自2004年开始(见例句.(36).最近AGASA协作[37]有降低能量下降10%左右我们的预测.但不明白专业的东西

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