Zobrazeno 1 - 10
of 1 124
pro vyhledávání: '"forbush decrease"'
Autor:
Starodubtsev S. A., Shadrina L. P.
Publikováno v:
Solar-Terrestrial Physics, Vol 10, Iss 3, Pp 50-57 (2024)
We analyze strong space weather disturbances during first ten days of September 2017, using the geomagnetic Dst index, parameters of normals to interplanetary shock fronts, direct measurements of interplanetary magnetic field, solar wind, and cosmic
Externí odkaz:
https://doaj.org/article/3111c5cf020e4643bc36c25ed62264e5
Autor:
Ogochukwu C Nwuzor, Austin Ojobeagu, Augustine Chikwendu, Patricia Otah, Cyril Ozibo, Chukwuemeka Nwaevo
Publikováno v:
Physics Access, Vol 4, Iss 2, Pp 49-58 (2024)
This study investigated the role of solar wind disturbances on variations in cosmic ray intensity. To conduct the study, use was made of the data on cosmic rays from the SOPO, CLMX, and MOSC neutron stations, as well as solar wind speed data from 2
Externí odkaz:
https://doaj.org/article/dc4c62b9fe52409bba84fb860183b53d
Autor:
Ugwu, Chukwuebuka J. a, b, ⁎, Alhassan, Jibrin A. c, Okike, Ogbonnaya d, Menteso, Firew M. c, e, Ugwu, Ngozi M. c, Chukwude, Augustine E. c, Iyida, Evaristus U. c, Eya, Innocent O. a, Ugwoke, Romanus E. f, Obiegbuna, Dominic C. a, Odo, Finbar C. c, Orji, Orji P. c
Publikováno v:
In Advances in Space Research 1 January 2025 75(1):1354-1370
Autor:
Sierra-Porta, D.
Publikováno v:
In Chaos, Solitons and Fractals: the interdisciplinary journal of Nonlinear Science, and Nonequilibrium and Complex Phenomena August 2024 185
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 2, Pp 94-100 (2023)
Diffusion and electromagnetic mechanisms determine the formation of sporadic Forbush decreases. The diffusion mechanism affects the Forbush decrease amplitude in the turbulent layer, and the part of the coronal mass ejection preceding the magnetic cl
Externí odkaz:
https://doaj.org/article/a9981d17877f43a690a6cc949115bf0c
Autor:
Natalya Kilifarska, Klaudio Peqini
Publikováno v:
Earth and Space Science, Vol 10, Iss 7, Pp n/a-n/a (2023)
Abstract The sensitivity of atmospheric ozone to geomagnetic storms and reduced cosmic rays' (CRs) intensity (called Forbush decrease [FD]) has been noticed for many years. However, it is still unclear what the factors affecting ozone density are—w
Externí odkaz:
https://doaj.org/article/246847d78b9446ad8a15722c1a7a24a9
Publikováno v:
Results in Physics, Vol 43, Iss , Pp 106076- (2022)
The Forbush effect is one of the striking examples of irregular variations in the cosmic ray (CR) flux. It is a heliospheric phenomenon that includes a decrease and a recovery of the CR intensity and small changes in the CR density and anisotropy bef
Externí odkaz:
https://doaj.org/article/0ad5c26a0b484ad8b0589acca8ebb7a3
Akademický článek
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Akademický článek
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Autor:
Ashot Chilingarian
Publikováno v:
Atmosphere, Vol 14, Iss 2, p 300 (2023)
High-energy physics in the atmosphere (HEPA) has undergone an intense reformation in the last decade. Correlated measurements of particle fluxes modulated by strong atmospheric electric fields, simultaneous measurements of the disturbances of the nea
Externí odkaz:
https://doaj.org/article/7a370b9651e447c4b3ec22caa299dca6