Primary Particle Energy Calibration of the EAS Radio Pulse Height

Primary Particle Energy Calibration of the EAS Radio Pulse Height
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EAS 无线电脉冲高度的一次粒子能量校准

DOI：
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发表时间：
2008
期刊：
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影响因子：
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通讯作者：
Ensus
Ensus
中科院分区：
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文献类型：
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作者：
H. A.;Orneffer;A. J.C.;Rteaga;A. J.;Uffenberg;B. F.;Adea;B. L.;Ähren;B. K.;Ekk;B. M.;Ertaina;B. P.L.;Iermann;B. J.;Lümer;B. H.;Ozdog;B. I.M.;Rancus;Rüggemann;B. P.;uchholz;B. S.;Uitink;Utcher;C. A.;Hiavassa;C. F.;Ossavella;D. K.;Aumiller;V.;De;ouza;E. R.;ngel;F. H.;Alcke;G. H.;Emmeke;G. P.L.;Hia;G. R.;Lasstetter;G. C.;Rupen;Aungs;H. D.;Eck;H. J.R.;Örandel;H. T.;Uege;I. P.G.;Sar;K. K.;Ampert;K. D.;Ickelbick;K. Y.;Olotaev;K. O.;Römer;K. J.;Uijpers;L. S.;Afebre;L. P.;uczak;M. H.J.;Athes;Ayer;M. C.;Eurer;M. J.;Ilke;M. B.;Itrica;Orello;N. G.;Avarra;N. S.;Ehls;N. A;Igl;O. J.;Ehlschläger;O. S.;Stapchenko;P. M.;Etcu;P. J.;etrovic;P. T.;Ierog;P. S;Lewnia;R. J.;Autenberg;R. H.;Ebel;S. H;Chieler;S. O;Ima;S. K.;Ingh;S. M.;Tümpert;T. G.C.;Rinchero;U. H.;Lrich;J.;Van;Uren;W. W.;Alkowiak;W. A.;Eindl;W. J.;Ochele;Z. J.;Abierowski;Z. J.A.;Ensus

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LOPES是用数字无线电接收器测量空气簇射的无线电发射的开创性实验。它设置在KA SCADE-Grande空气簇射阵列的现场，并与之联合采集数据，这为联合收割机LOPES和KASCADE-Grande数据的联合提供了独特的可能性。在第一阶段，LOPES由放置在KASCADE阵列内的10个天线组成。在其第二阶段，它已扩展到30个天线，这增加了良好重建的事件的检测率。此外，一个新的，绝对校准的无线电天线现在可用。通过将测量的射电脉冲高度与KASCADE-Grande测量的空气簇射参数相关联，导出了描述射电脉冲高度与空气簇射几何和初级粒子能量的关系式。从而使我们能够从无线电数据中估计宇宙射线的能量。
LOPES is the pioneering experiment for the measurement of ra dio emission from air showers with digital radio receivers. It is set up at the site of the KA SCADE-Grande air shower array and takes data in conjunction with it. This gives the unique possibili ty to combine LOPES and KASCADE-Grande data. In the first phase LOPES consisted of 10 antennas placed inside the KASCADE array. In its second phase it has been extended to 30 antennas, which increases th e detection rate of well reconstructed events. Also a new, absolute calibration of the radio antennas is now available. By correlating the measured radio pulse height with air shower parameters measured by KASCADE -Grande, we have derived a formula that describes the radio pulse height as a function of air shower g eometry and primary particle energy. Thus allowing us to estimate the cosmic ray energy from radio data .