Lunar Space Missions for Ultrahigh-energy Cosmic Rays and Neutrinos Observation

被引：1
作者：
Gusev, G. A. [1 ]
Chechin, V. A. [1 ]
Ryabov, V. A. [1 ]
机构：
[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 119991, Russia
来源：
5TH INTERNATIONAL WORKSHOP ON ACOUSTIC AND RADIO EEV NEUTRINO DETECTION ACTIVITIES (ARENA 2012) | 2013年 / 1535卷
关键词：
GZK cut-off; ultrahigh-energy particles; radio detector; regolith; Vavilov-Cherenkov radiation; multi-satellite lunar systems;
D O I：
10.1063/1.4807517
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Two stages of exploring the lunar surface as a target for the interaction of ultrahigh-energy cosmic rays and neutrinos are discussed. The first step is connected with the Lunar Orbital Radio Detector (LORD) experiment in the space mission Luna-Glob, scheduled for the near future. The current status of the LORD instrument development is represented. The aperture of the lunar orbital radio detector exceeds all existing ground-based detector arrays. Successful completion of the LORD experiment will permit to consider the second step of the program namely multi-satellite lunar systems to increase the statistics and the accuracy of the experiment.
引用
收藏
页码：37 / 40
页数：4
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