scholarly journals Simulations of Muon Flux in Slanic Salt Mine

2012 ◽  
Vol 2012 ◽  
pp. 1-8 ◽  
Author(s):  
Mehmet Bektasoglu ◽  
Halil Arslan ◽  
Denis Stanca

Geant4 simulation package was used to simulate muon fluxes at different locations, the floor of UNIREA mine and two levels of CANTACUZINO mine, of Slanic Prahova site in Romania. This site is specially important since it is one of the seven sites in Europe that are under consideration of housing large detector components of Large Apparatus studying Grand Unification and Neutrino Astrophysics (LAGUNA) project. Simulations were performed for vertical muons and for muons with a zenith angleθ≤60°. Primary muon flux and energies at ground level were obtained from previous measurements. Results of the simulations are in general agreement with previous simulations made using MUSIC simulation program and with the measurements made using a mobile detector.

1995 ◽  
Vol 05 (04) ◽  
pp. 669-697 ◽  
Author(s):  
ROMUALD SZCZESNY ◽  
MIECZYSLAW RONKOWSKI

The methods, models and techniques — presented in the companion paper — have been used as a basis for the evaluation of popular general-purpose electrical circuit simulation programs, in particular, their applicability in the analysis of power electronic circuits. As a result of this critical evaluation, the general requirements for the simulation program adequate for converter systems studies and design have been formulated. On this basis the algorithm of TCAD — a general-purpose converter system simulation program — has been elaborated. In presentation of the TCAD program three parties have been distinguished: the first one emphasizes the applications of modern simulation methods for converter systems, the second describes briefly the features of the main modules of the TCAD package, and the third presents some simulation examples of practical converter systems. Three simulation examples are presented: two resonant converters and an induction motor drive fed by a full-bridge voltage source PWM inverter at normal and fault operation conditions. A good agreement between simulation and experimental results has proved that this simulation package is a power tool for research, teaching and engineering practice.


2013 ◽  
Vol 2013 ◽  
pp. 1-4 ◽  
Author(s):  
Halil Arslan ◽  
Mehmet Bektasoglu

Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standard rock have been investigated using Geant4 simulation package. Muons with energies above 100 GeV were distributed from the ground level taking into account the muon charge ratio of~1.3 at sea level. The simulated differential muon intensities are in good agreement with the intensities given in the literature. Furthermore, the simulation results for the integrated intensities are consistent with the experimental data, particularly at depths above 4000 m.w.e., where the simulation gives slightly smaller intensities than the experimental ones. In addition, the simulated exponentnat different underground depths agrees well with the experimental points, especially above~2000 m.w.e.


2005 ◽  
Vol 20 (29) ◽  
pp. 6950-6952 ◽  
Author(s):  
T. DJEMIL ◽  
R. ATTALLAH ◽  
J. N. CAPDEVIELLE

We present in this paper the results of 3D-calculation of the atmospheric muon flux at different altitudes. We have used for this purpose the extensive air shower simulation package CORSIKA (v. 6.031) in combination with the hadronic interaction models VENUS (v. 4.12) at high energy (beyond 80 GeV) and GHEISHA (v. 2002) and UrQMD (v. 1.1) at lower energy. Our results are compared to data from different experiments (CAPRICE, BESS and HEAT). The correlation of the atmospheric muon flux to the primary zenith angle and primary energy is also investigated.


2020 ◽  
Vol 63 (6) ◽  
Author(s):  
Alejandra Vesga-Ramírez ◽  
David Sierra Porta ◽  
Jesús Peña Rodríguez ◽  
José Sanabria-Gómez ◽  
Martha Valencia-Otero ◽  
...  

By using a very detailed simulation scheme, we have calculated the cosmic ray background flux at 13 active Colombian volcanoes and developed a methodology to identify the most convenient places for a muon telescope to study their inner structure. Our simulation scheme considers three critical factors with different spatial and time scales: the geo-magnetic effects, the development of extensive air showers in the atmosphere, and the detector response at ground level. The muon energy dissipation along the path crossing the geological structure is modeled considering the losses due to ionization, and also contributions from radiative Bremßtrahlung, nuclear interactions, and pair production. By examining each particular volcano topography and assuming reasonable statistics for different instrument acceptances, we obtained the muon flux crossing each structure and estimated the exposure time for our hybrid muon telescope at several points around each geological edifice. After a detailed study from the topography, we have identified the best volcano to be studied, spotted the best points to place a muon telescope and estimated its time exposures for a significant statistics of muon flux. We have devised a mix of technical and logistic rules –the “rule of thumb” criteria– and found that only Cerro Machín, located at the Cordillera Central (4°29'N 75°22'W), can be feasibly studied today through muography. Cerro Negro and Chiles could be good candidates shortly.


2009 ◽  
Vol 2 (4) ◽  
pp. 1537-1573 ◽  
Author(s):  
I. Trebs ◽  
B. Bohn ◽  
C. Ammann ◽  
U. Rummel ◽  
M. Blumthaler ◽  
...  

Abstract. Representative values of the atmospheric NO2 photolysis frequency, (j(NO2)), are required for the adequate calculation and interpretation of NO and NO2 concentrations and exchange fluxes near the surface. Direct measurements of j(NO2) at ground level are often not available in field studies. In most cases, modeling approaches involving complex radiative transfer calculations are used to estimate j(NO2) and other photolysis frequencies for air chemistry studies. However, important input parameters for accurate modeling are often missing, most importantly with regard to the radiative effects of clouds. On the other hand, solar global irradiance ("global radiation", G) is nowadays measured as a standard parameter in most field experiments and in many meteorological observation networks around the world. A linear relationship between j(NO2) and G was reported in previous studies and has been used to estimate j(NO2) from G in the past 30 years. We have measured j(NO2) using spectro- or filter radiometers and G using pyranometers side-by-side at several field sites. Our results cover a solar zenith angle range of 0–90°, and are based on nine field campaigns in temperate, subtropical and tropical environments during the period 1994–2008. We show that a second-order polynomial function (intercept=0): j(NO2)=(1+α)×(B1×G+B2×G2), with α defined as the site-dependent UV-A surface albedo and the polynomial coefficients (including uncertainty ranges): B1=(1.47±0.03)×10−5 W−1 m2 s−1 and B2=(−4.84±0.31)×10−9 W−2 m4 s−1 can be used to estimate ground-level j(NO2) directly from G, independent of solar zenith angle under all atmospheric conditions. The absolute j(NO2)↓ residual of the empirical function is ±6×10−4 s−1 (95.45% confidence level). The relationship is valid for sites below 800 m a.s.l. and under low background albedo conditions. It is not valid in alpine regions, above snow or ice and sandy or dry soil surfaces. Our function can be applied to estimate chemical life times of the NO2 molecule with respect to photolysis, and is useful for surface-atmosphere exchange and photochemistry studies close to the ground, e.g., above fields with short vegetation and above forest canopies.


2012 ◽  
Vol 381 ◽  
pp. 012051 ◽  
Author(s):  
P Papadakis ◽  
D M Cox ◽  
J Konki ◽  
P A Butler ◽  
P T Greenlees ◽  
...  

2016 ◽  
Vol 43 (10) ◽  
pp. 298-301
Author(s):  
E. I. Yakovleva ◽  
V. A. Khomyakov ◽  
S. S. Khokhlov

2018 ◽  
Vol 2018 ◽  
pp. 1-11
Author(s):  
G. Aydın

The scintillating properties of active materials used in high energy and particle physics experiments play an important role regarding the performances of both calorimeters and experiments. Two scintillator materials, a scintillating glass and an inorganic crystals, were examined to be used for collider experiments showing good optical and scintillating properties. This paper discusses the simulated performances of two materials of interest assembled in a scintillator-photodetector combination. The computational study was carried out with Geant4 simulation program to determine energy resolutions of such calorimeter with different beam energies and calorimeter sizes.


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