Zobrazeno 1 - 10
of 121
pro vyhledávání: '"Yu. I. Yermolaev"'
Publikováno v:
Annales Geophysicae, Vol 28, Pp 2177-2186 (2010)
A comparison of specific interplanetary conditions for 798 magnetic storms with Dst
Externí odkaz:
https://doaj.org/article/a6f47332c7fc49b381666cd158a65f03
Publikováno v:
Cosmic Research. 60:452-460
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b77a46e70114af655cba68af10840f37
https://doi.org/10.1134/s0010952522060053
https://doi.org/10.1134/s0010952522060053
Publikováno v:
Geomagnetism and Aeronomy. 62:505-513
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eee7193a4e7c8bd68acecbf8d1c085ac
https://doi.org/10.1134/s0016793222050103
https://doi.org/10.1134/s0016793222050103
Publikováno v:
Cosmic Research. 60:67-72
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75481e8e613ff4fbe52feaa3591a939d
https://doi.org/10.1134/s0010952522020046
https://doi.org/10.1134/s0010952522020046
Publikováno v:
Cosmic Research. 59:415-426
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::595a5c465b947bb6a8df33369e3fb8bf
https://doi.org/10.1134/s0010952521060022
https://doi.org/10.1134/s0010952521060022
Publikováno v:
Geomagnetism and Aeronomy. 61:666-677
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb6ab0e74d0b2a1ed4e298eaff2766c7
https://doi.org/10.1134/s0016793221050042
https://doi.org/10.1134/s0016793221050042
Publikováno v:
Geomagnetism and Aeronomy. 61:696-702
Abstract The bow shock crossing by the solar wind can lead in a number of cases to significant changes in the development of the turbulent cascade. Individual cases previously studied on the basis of experimental measurements of the characteristics o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1cc854ad05196fef737d83481ef85d22
https://doi.org/10.1134/s0016793221050108
https://doi.org/10.1134/s0016793221050108
Publikováno v:
Cosmic Research. 58:492-500
One perturbed type of solar wind and magnetospheric disturbance drivers is the compression region in front of fast ICMEs—the Sheath region. In front of this region, an interplanetary shock is observed in approximately half of cases. However, the pa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d9345151557e5e656785f4ce47d1942c
https://doi.org/10.1134/s0010952520060052
https://doi.org/10.1134/s0010952520060052
Publikováno v:
Cosmic Research. 58:450-459
The structure of interplanetary shock fronts was studied based on the data from the BMSW plasma spectrometer, installed on the SPEKTR-R spacecraft, supplemented by magnetic field measurements on the WIND spacecraft. Special attention was paid to peri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b173b5272af5cdf148fa71449da7152b
https://doi.org/10.1134/s0010952520060015
https://doi.org/10.1134/s0010952520060015
Autor:
Yu. I. Yermolaev, Maria Riazantseva, L. S. Rakhmanova, Irina Lodkina, G. N. Zastenker, L. S. Chesalin
Publikováno v:
Cosmic Research. 58:468-477
This work is devoted to the study of properties of spectra of turbulent solar wind fluctuations in plasma compression regions, such as CIR (the plasma compression regions in front of high-speed streams from coronal holes) and SHEATH (the compression
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::36a109589b0b919151dfd81e3e9bbb4a
https://doi.org/10.1134/s001095252006009x
https://doi.org/10.1134/s001095252006009x