Cosmic rays muon flux measurements at Belgrade shallow underground laboratory

2015 ◽  
Author(s):  
N. Veselinović ◽  
A. Dragić ◽  
D. Maletić ◽  
D. Joković ◽  
M. Savić ◽  
...  
2019 ◽  
Author(s):  
F. Ludwig ◽  
L. Wagner ◽  
T. Al-Abdullah ◽  
D. Bemmerer ◽  
K. Zuber

2014 ◽  
Vol 9 (08) ◽  
pp. P08010-P08010 ◽  
Author(s):  
L N Kalousis ◽  
E Guarnaccia ◽  
J M Link ◽  
C Mariani ◽  
R Pelkey

2020 ◽  
Author(s):  
Ziyi 郭子溢 Guo ◽  
Shaomin 陈少敏 Chen ◽  
zhe wang ◽  
Minfang Yeh ◽  
Linyan Wan ◽  
...  

Author(s):  
M Robinson ◽  
V.A Kudryavtsev ◽  
R Lüscher ◽  
J.E McMillan ◽  
P.K Lightfoot ◽  
...  

2013 ◽  
Vol 2013 ◽  
pp. 1-7 ◽  
Author(s):  
B. Mitrica ◽  
D. Stanca ◽  
M. Petcu ◽  
I. M. Brancus ◽  
R. Margineanu ◽  
...  

Precise measurements of the muon flux are important for different practical applications, both in environmental studies and for the estimation of the water equivalent depths of underground sites. A mobile detector for cosmic muon flux measurements has been set up at IFIN-HH, Romania. The device is used to measure the muon flux on different locations at the surface and underground. Its first configuration, not used in the present, has been composed of two 1 m2scintillator plates, each viewed by wave length shifters and read out by two Photomultiplier Tubes (PMTs). A more recent configuration, consists of two 1 m2detection layers, each one including four 1 · 0,25 m2large scintillator plates. The light output in each plate is collected by twelve optical fibers and then read out by one PMT. Comparative results were obtained with both configurations.


Author(s):  
T. Enqvist ◽  
A. Mattila ◽  
V. Föhr ◽  
T. Jämsén ◽  
M. Lehtola ◽  
...  

Author(s):  
Francesco Nozzoli ◽  
Cinzia Cernetti

Cosmic Rays (CR) are a powerful tool for the investigation of the structure of the magnetic fields in the galactic halo and the property of the Inter-Stellar Medium. Two parameters of the CR propagation models: the galactic halo thickness, H, and the diffusion coefficient, D, are loosely constrained by current CR flux measurements, in particular a large degeneracy exist being only H/D well measured. The 10Be/9Be isotopic flux ratio (thanks to the 2 My lifetime of 10Be) can be used as a radioactive clock providing the measurement of CR residence time in the galaxy. This is an important tool to solve the H/D degeneracy. Past measurements of 10Be/9Be isotopic flux ratio in CR are scarce, limited to low energy and affected by large uncertainties. Here a new technique to measure 10Be/9Be isotopic flux ratio, with a Data-Driven approach, in magnetic spectrometers is presented. As an example by applying the method to Beryllium events published by PAMELA experiment it is now possible to determine the important 10Be/9Be measurement avoiding the prohibitive uncertainties coming from the Monte Carlo simulation. It is shown how the accuracy of PAMELA data permits to infer a value of the halo thickness H within 25% precision.


2019 ◽  
Author(s):  
T. Hensel ◽  
M. Grieger ◽  
J. Agramunt ◽  
J. L. Taín ◽  
D. Bemmerer ◽  
...  

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