Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Yu. N. Mishutina"'
Autor:
V. E. Chinkin, V. G. Getmanov, I. V. Yashin, V. V. Shutenko, E. I. Yakovleva, Yu. N. Mishutina, A. N. Dmitrieva, A. A. Kovylyaeva, Alexander Soloviev, M. N. Dobrovolsky, N. S. Barbashina
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:464-467
Forbush effects caused by powerful X-class solar flares are studied using URAGAN muon hodoscope data for the period 2007–2019. The URAGAN muon hodoscope registers the cosmic ray muon flux on the Earth’s surface from different directions simultane
Publikováno v:
Physics of Atomic Nuclei. 83:294-299
Variations of secondary cosmic rays on the Earth’s surface depend on the solar activity. To study these variations, neutron monitors and muon detectors are used. Observations of muons and hadrons complement each other in terms of the energies of th
Autor:
V. G. Getmanov, Igor Yashin, A.G. Gvishiani, A. A. Kovylyaeva, V. V. Shutenko, Yu. N. Mishutina, I. I. Astapov, A.G. Gvishian, A. N. Dmitrieva, Alexander Soloviev
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Autor:
V. V. Borog, A. A. Petrukhin, I. I. Yashin, A. A. Kovylyaeva, V. V. Shutenko, N. S. Barbashina, A. N. Dmitrieva, E. I. Yakovleva, I. I. Astapov, Yu. N. Mishutina, K. G. Kompaniets
Publikováno v:
Physics of Atomic Nuclei. 82:892-896
Results of the study of variations of cosmic ray muon flux at the Earth surface during Forbush decreases registered in 2007–2018 by means of the muon hodoscope URAGAN are presented. The dynamics of the amplitude spectral index at different stages (
Autor:
A. Yu. Konovalova, Yu. N. Mishutina, N. S. Barbashina, I. I. Yashin, N. V. Osetrova, V. V. Shutenko, I. I. Astapov
Publikováno v:
Physics of Atomic Nuclei. 82:909-915
The influence of a high-speed solar wind on the state of magnetosphere, as well as on the cosmic ray flux registered on the Earth’s surface by the muon hodoscope URAGAN (MEPhI) is discussed. The results of the analysis of the parameters of muon flu
Autor:
R. V. Sidorov, Sh. R. Bogoutdinov, I. S. Veselovsky, A. D. Gvishiani, Yu. N. Mishutina, V. V. Shutenko, A. A. Solov’ev, I. I. Astapov, I. I. Yashin, N. V. Osetrova, A. N. Dmitrieva, V. V. Borog, V. G. Getmanov, N. S. Barbashina, A. A. Petrukhin
Publikováno v:
Physics of Atomic Nuclei. 81:1370-1373
Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually car
Autor:
K. G. Kompaniets, A. A. Petrukhin, V. V. Borog, Yu. N. Mishutina, E. I. Yakovleva, A. N. Dmitrieva, N. S. Barbashina, I. I. Astapov, V. V. Shutenko, I. I. Yashin, A. A. Kovylyaeva
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:563-565
Results are presented from an analysis of changes in the muon flux of cosmic rays during Forbush effects, recorded by the URAGAN muon hodoscope in the period 2012–2017 and the scintillation muon hodoscope in 2016–2017. Characteristics of the Forb
Autor:
A. Chiavassa, A. G. Bogdanov, E A Zadeba, A. N. Dmitrieva, E. A. Yurina, G. Mannocchi, I. I. Astapov, Yu. N. Mishutina, A. Yu. Konovalova, V. V. Shutenko, S. S. Khokhlov, K. O. Yurin, V. V. Ovchinnikov, R. P. Kokoulin, V. V. Borog, I. A. Shulzhenko, Gian Carlo Trinchero, M. B. Amelchakov, Yu. V. Stenkin, V. S. Vorobiev, N. S. Barbashina, V. V. Kindin, K. G. Kompaniets, D. M. Gromushkin, I. I. Yashin, F. A. Bogdanov, A. A. Kovylyaeva, A. A. Petrukhin
Publikováno v:
Journal of Instrumentation. 16:T08014
Autor:
I. I. Astapov, N. S. Barbashina, Z. T. Izhbulyakova, D. M. Gromushkin, L. Bouchama, A. N. Dmitrieva, F. A. Bogdanov, Yu. N. Mishutina, A. A. Kovylyaeva
Publikováno v:
Journal of Physics: Conference Series. 1690:012012
The experimental data on thermal neutron flux registered by the “Neutron” setup (MEPhI, Moscow) on the Earth's surface for the period from May 2015 to February 2019 were analyzed. The effects of Forbush decrease (FD) and the lunar cycles were stu
Autor:
N. S. Barbashina, K. G. Kompaniets, I. I. Astapov, A. N. Dmitrieva, Yu. N. Mishutina, V. V. Shutenko, V. V. Borog, I. I. Yashin, E. I. Yakovleva, A. A. Petrukhin, R. P. Kokoulin, D. V. Chernov
Publikováno v:
Advances in Space Research. 56:2693-2705
Muon hodoscope URAGAN continuously detects the angular distribution of muons in a wide range of zenith angles and allows to obtain information about the variations both in the intensity and angular characteristics of the muon flux related with active