Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Vladislav Chinkin"'
Autor:
Victor Getmanov, Vladislav Chinkin, Roman Sidorov, Alexei Gvishiani, Mikhail Dobrovolsky, Anatoly Soloviev, Anna Dmitrieva, Anna Kovylyaeva, Nataliya Osetrova, Igor Yashin
Publikováno v:
Applied Sciences, Vol 11, Iss 10, p 4524 (2021)
Problems of digital processing of Poisson-distributed data time series from various counters of radiation particles, photons, slow neutrons etc. are relevant for experimental physics and measuring technology. A low-pass filtering method for normalize
Externí odkaz:
https://doaj.org/article/4013089bae7345d6a6f2f9ac1cd3958e
Autor:
Vladislav Chinkin, R. A. Sidorov, A. A. Kovylyaeva, Victor Getmanov, M. N. Dobrovolsky, I. I. Yashin, A. N. Dmitrieva, Nataliya Osetrova, Alexei Gvishiani, Anatoly Soloviev
Publikováno v:
Applied Sciences, Vol 11, Iss 4524, p 4524 (2021)
Applied Sciences
Volume 11
Issue 10
Applied Sciences
Volume 11
Issue 10
Problems of digital processing of Poisson-distributed data time series from various counters of radiation particles, photons, slow neutrons etc. are relevant for experimental physics and measuring technology. A low-pass filtering method for normalize
Autor:
R. V. Sidorov, Vladislav Chinkin, Leonid Tsibizov, I. I. Yashin, A. D. Gvishiani, N. V. Osetrova, A. A. Kovylyaeva, Michael Dobrovolsky, Victor Getmanov, Anatoly Soloviev, A. N. Dmitrieva
Muon flux intensity modulation (MFIM) recognition is a relevant solar-terrestrial physics problem. The MFIM discussed are due to geoeffective solar coronal mass ejections.The necessary observations are carried out using a computerized muon hodoscope
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46ac8a171d17a70052e9f07297a50bf5
https://doi.org/10.5194/egusphere-egu21-303
https://doi.org/10.5194/egusphere-egu21-303
Autor:
Vladislav Chinkin, Anatoly Soloviev, A. D. Gvishiani, A. N. Dmitrieva, V. G. Getmanov, A. A. Kovylyaeva, I. I. Yashin, M. N. Dobrovolsky, N. V. Osetrova, R. V. Sidorov
Muon flux intensity modulation (MFIM) recognition is a relevant solar-terrestrial physics problem. The considered MFIM, recorded on the Earth's surface, are caused by extreme heliospheric events – the geoeffective solar coronal mass ejections.The U
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8da6986c658f7ee7e21cb6831418833b
https://doi.org/10.5194/egusphere-egu21-310
https://doi.org/10.5194/egusphere-egu21-310