排序方式: 共有18条查询结果,搜索用时 0 毫秒
1.
R. P. Kokoulin A. G. Bogdanov D. M. Gromushkin G. Mannocchi A. A. Petrukhin O. Saavedra N. V. Tolkacheva G. Trinchero D. V. Chernov V. V. Shutenko I. I. Yashin 《Bulletin of the Russian Academy of Sciences: Physics》2011,75(3):395-398
Characteristics of muon bundles detected with the DECOR detector are compared to predictions based on different hadron interaction models and various assumptions as to the spectrum and mass composition of primary cosmic rays. The intensity of primary cosmic rays derived from the muon bundle data is considerably higher than that measured by means of the fluorescence technique. Either changes in the hadron interaction characteristics at ultrahigh energies or a revision of the energy calibration in the fluorescence technique of measuring EAS energy is required to explain these results. 相似文献
2.
V. V. Alekseenko D. M. Gromushkin Yu. V. Sten’kin 《Bulletin of the Russian Academy of Sciences: Physics》2011,75(6):857-859
Thermal neutron fluxes were measured using two types of scintillation detectors based on the inorganic scintillator ZnS(Ag):
6LiF+ZnS(Ag) and 10B2O3 + KCl+ZnS(Ag). The preliminary results from these measurements are given. The thermal neutron concentration as a function
of altitude above sea level was determined. The measurements were performed at three locations: in Moscow, at the Baksan Neutrino
Observatory of the Russian Academy of Sciences, and at the Gran Sasso National Laboratory. Variations of neutron count rates
associated with lunar cycles were observed at the remote laboratories. 相似文献
3.
Kuzmenkova P. S. Gromushkin D. M. Shulzhenko I. A. Tretyakova T. D. 《Physics of Atomic Nuclei》2021,84(9):1588-1592
Physics of Atomic Nuclei - The paper presents a comparison of three neutrons identifying methods in scintillators based on ZnS with 6Li and 10B: charge integration method, pulse gradient analysis,... 相似文献
4.
Shchegolev O. B. Bogdanov F. A. Izhbulyakova Z. T. Gromushkin D. M. Stenkin Yu. V. 《Physics of Atomic Nuclei》2020,83(2):290-293
Physics of Atomic Nuclei - PRISMA-32 (PRImary Spectrum Measurement Array) is working since 2012 in the Scientific & Educational Center NEVOD (NRNU ‘‘MEPhI’’,... 相似文献
5.
D. M. Gromushkin Yu. V. Sten’kin I. B. Khatsukov 《Bulletin of the Lebedev Physics Institute》2010,37(11):344-346
The applicability of new-type unshielded detectors based on zinc sulfide ZnS(Ag) and lithium fluoride enriched with 6Li isotope to 90% to thermal neutron measurements is demonstrated. The results of measurements of the thermal neutron counting
rate and flux near the Earth’s surface are presented. The existence of the concentration gradient of thermal neutrons near
the Earth’s surface at placing the counter at the various levels (from −4 to 10.5 m) in an experimental building is shown.
The effect of meteoparameters on the counting rate of thermal neutrons for a long time is shown. 相似文献
6.
D. M. Gromushkin A. A. Petrukhin Yu. V. Stenkin I. I. Yashin 《Bulletin of the Russian Academy of Sciences: Physics》2011,75(3):374-376
Experimental data on detecting the thermal neutrons that accompany extensive air showers (EAS) over a long period of time
(May 2009–April 2010) are presented. The data were obtained by means of prototype for an innovative new array (PRISMA) for
EAS study. The workability of this array and its ability to yield completely new information on the hadron and electron components
of EAS was checked experimentally over long period of time (in the minimal version of the prototype). 相似文献
7.
8.
The results of Monte-Carlo simulations of extensive air showers are presented to show the difference of the hadronic component content at various altitudes with the aim to choose an optimal altitude for a PRISMA-like experiment. The CORSIKA program for EAS simulations with QGSJET and GHEISHA models was used to calculate the number of hadrons reaching the observational level inside a circle of 50 m radius around the EAS axis. Then the number of neutrons produced by the hadronic component was calculated using an empirical relationship between the two components. We have tested the results with the ProtoPRISMA array at sea level, and recorded the neutrons which are consistent with the simulation results. 相似文献
9.
A. G. Bogdanov D. M. Gromushkin R. P. Kokoulin G. Mannocchi A. A. Petrukhin O. Saavedra G. Trinchero D. V. Chernov V. V. Shutenko I. I. Yashin 《Physics of Atomic Nuclei》2010,73(11):1852-1869
A new method for studying extensive air showers is considered. The method is based on the phenomenology of the localmuon density.
It is shown that measurement ofmuon-density spectra at various zenith angles makes it possible to obtain information about
the energy spectrum, mass composition, and interaction of cosmic rays over a broad range of energies (1015–1018 eV) by using a single array of comparatively small size. The results obtained from a comparison of experimental data on muon
bundles from the DECOR coordinate detector with the results of simulation performed under various assumptions on the properties
of the primary flux and for various hadron-interaction models are presented, and possible versions of the interpretation of
these results are discussed. 相似文献
10.
I. I. Yashin N. S. Barbashina A. G. Bogdanov D. M. Gromushkin A. N. Dmitrieva V. V. Kindin R. P. Kokoulin K. G. Kompaniets G. Mannocchi A. A. Petrukhin O. Saavedra D. A. Timashkov G. Trinchero D. V. Chernov V. V. Shutenko 《Bulletin of the Russian Academy of Sciences: Physics》2007,71(4):556-559
The results of investigation of muon bundles at the Earth’s surface in a wide range of zenith angles on the basis of the new phenomenological characteristic of extensive air showers—spectra of local muon density—have been investigated. Features of the local-density spectra are considered within a simple analytical model. The expected distributions of muon density in a wide range of zenith angles and primary energies, calculated on the basis of the CORSIKA code, are compared with the experimental data. 相似文献