Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Sergey Lunyushkin"'
Publikováno v:
Solar-Terrestrial Physics, Vol 7, Iss 2, Pp 57-69 (2021)
The ground-based automatic method for determining auroral oval (AO) boundaries developed by the authors [Lunyushkin, Penskikh, 2019] has been modified and expanded to the Southern Hemisphere. Input data of the method contains large-scale distribution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7cad6ca0966fa36e2c0c80ee2ffef80c
https://naukaru.ru/en/nauka/article/42243/view
https://naukaru.ru/en/nauka/article/42243/view
Publikováno v:
Solar-Terrestrial Physics, Vol 7, Iss 1, Pp 32-40 (2021)
We continue to study the physical processes occurring during the August 17, 2001 magnetospheric storm by analyzing the dynamics of the intensity of field-aligned currents (FACs) in Iijima—Potemra Region 1 in the polar ionospheres of the two hemisph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52976253e42e0c4a2d2845e9f090d48a
https://doi.org/10.12737/szf-71202104
https://doi.org/10.12737/szf-71202104
Autor:
Sergey Lunyushkin, Yury Penskikh
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 2, Pp 88-100 (2019)
It is shown that the convection reversal boundary is a fundamental parameter of the magnetosphere-ionosphere coupling, which determines a strong analogy between the electrostatic potential of the ionosphere and the equivalent current function in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::180952deb8fc7665887361a768e66052
https://doi.org/10.12737/szf-52201913
https://doi.org/10.12737/szf-52201913
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 2, Pp 15-17 (2019)
The magnetogram inversion technique (MIT), developed at ISTP SB RAS more than forty years ago, has been used until recently only in the Northern Hemisphere. In recent years, MIT has been improved and extended to make instantaneous calculations of 2D
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::056cf69bb11ec17468e391ab3dc7a21b
https://doi.org/10.12737/stp-52201903
https://doi.org/10.12737/stp-52201903
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 2, Pp 33-38 (2019)
We analyze significant increases in 630 nm atomic oxygen night emissions during very strong geomagnetic storms, using optical measurements, theoretical modeling, and magnetogram inversion technique (MIT) data. It is shown that during strong magnetic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78ad3c1b6ff86b0f53d741a59ec8b93d
https://naukaru.ru/en/nauka/article/29448/view
https://naukaru.ru/en/nauka/article/29448/view