A cosmic-ray gas čerenkov counter with adjustable velocity threshold

1956 ◽  
Vol 4 (6) ◽  
pp. 1558-1564 ◽  
Author(s):  
E. J. Hanson ◽  
D. C. Moore
1963 ◽  
Vol 11 (2) ◽  
pp. 193-208
Author(s):  
L.V. Kurnosova ◽  
V.I. Logachev ◽  
L.A. Razorenov ◽  
M.I. Fradkin

1968 ◽  
Vol 46 (10) ◽  
pp. S805-S808 ◽  
Author(s):  
E. A. Bogomolov ◽  
V. K. Karakadko ◽  
N. D. Lubyanaya ◽  
V. A. Romanov ◽  
M. G. Totubalina ◽  
...  

The east–west asymmetry has been measured to obtain a more accurate value of the antiproton–proton flux ratio in the primary cosmic radiation. The measurements have been carried out at middle latitudes at a depth of 10 g/cm2 of atmosphere and at a zenith angle of 60°. The telescope used for detection consisted of two scintillation counters, a lucite Cerenkov counter, and a gas Cerenkov counter. The threshold of the gas Cerenkov detector has been changed from 1.7 BeV to 5.2 BeV (for protons) in flight. For orientation of the device in space the earth's magnetic field was used.The preliminary results of the experiment are given.


1982 ◽  
Vol 43 (C8) ◽  
pp. C8-69-C8-88 ◽  
Author(s):  
B. Rossi
Keyword(s):  

2010 ◽  
Vol 180 (5) ◽  
pp. 519 ◽  
Author(s):  
L.I. Dorman
Keyword(s):  

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