排序方式： 共有11条查询结果，搜索用时 15 毫秒
1.
2.
3.
4.
5.
6.
7.
8.
B. A. Khrenov V. V. Alexandrov D. I. Bugrov G. K. Garipov N. N. Kalmykov M. I. Panasyuk S. A. Sharakin A. A. Silaev I. V. Yashin V. M. Grebenyuk D. V. Naumov A. G. Olshevsky B. M. Sabirov R. N. Semenov M. Slunechka I. I. Skryl L. G. Tkatchev O. A. Saprykin V. S. Syromyatnikov V. E. Bitkin S. A. Eremin A. I. Matyushkin F. F. Urmantsev V. Abrashin V. Koval Y. Arakcheev A. Cordero O. Martinez E. Morena C. Robledo H. Salazar L. Villasenor A. Zepeda I. Park M. Shonsky J. Zicha 《Physics of Atomic Nuclei》2004,67(11):2058-2061
The KLYPVE space experiment has been proposed to study the energy spectrum, composition, and arrival direction of ultrahigh-energy cosmic rays (UHECR) by detecting from satellites the atmosphere fluorescence and scattered Cherenkov light produced by EAS, initiated by UHECR particles. The TUS setup is a prototype KLYPVE instrument. The aim of the TUS experiment is to detect dozens of UHECR events in the energy region of the GZK cutoff, to measure the light background, to test the atmosphere control methods, and to study stability of the optical materials, PMTs, and other instrumental parts in space environment. 相似文献
9.
P. A. Apanasevich V. N. Abrashin R. G. Zaporozhchenko V. A. Mukha 《Journal of Applied Spectroscopy》1988,49(5):1131-1135
Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 49, No. 5, pp. 761–766, November, 1988. 相似文献
10.