Zobrazeno 1 - 10
of 39
pro vyhledávání: '"N. L. Borodkova"'
Publikováno v:
Annales Geophysicae, Vol 30, Pp 1285-1295 (2012)
We performed global MHD simulations of the geosynchronous magnetic field in response to fast solar wind dynamic pressure (Pd) enhancements. Taking three Pd enhancement events in 2000 as examples, we found that the main features of the total field
Externí odkaz:
https://doaj.org/article/02331ab31809410a98a01fb9d8674a66
Autor:
N. L. Borodkova, A. G. Yahnin, K. Liou, J.-A. Sauvaud, A. O. Fedorov, V. N. Lutsenko, M. N. Nozdrachev, A. A. Lyubchich
Publikováno v:
Annales Geophysicae, Vol 20, Pp 341-347 (2002)
Interball-1 observations of a substorm development in the mid-tail on 16 December 1998 are compared with the auroral dynamics obtained from the Polar UV imager. Using these data, the relationship between plasma flow directions in the tail and t
Externí odkaz:
https://doaj.org/article/18b67ae57b784692a23a9ccc4b195863
Autor:
A. G. Yahnin, V. A. Sergeev, T. Bösinger, T. I. Sergienko, I. A. Kornilov, N. L. Borodkova, M. F. Thomsen, R. D. Belian, J.-A. Sauvaud, V. N. Lutsenko, A. A. Skalsky
Publikováno v:
Annales Geophysicae, Vol 19, Pp 687-698 (2001)
We study the isolated substorm that occurred after a long quiet period, which showed all of the substorm signatures except for the first half hour of the expansion phase, which could be characterized as a pseudobreakup sequence, rather than a
Externí odkaz:
https://doaj.org/article/9ad1ff5564194c86b7b51c0393ee2b2d
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:
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:
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
Publikováno v:
Geomagnetism and Aeronomy. 60:708-713
The variations in the parameters of twice ionized helium ions He++ of solar wind plasma during the passage of the front of the interplanetary shock are studied. Data taken from measurements by the Bright Monitor of Solar Wind (BMSW) installed onboard
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::60b08d868141495366bb759bf459700b
https://doi.org/10.1134/s0016793220060122
https://doi.org/10.1134/s0016793220060122
Publikováno v:
Geomagnetism and Aeronomy. 58:728-736
Data from the Fast Solar Wind Monitor (BMSW) of the science payload onboard the SPEKTR-R satellite and data from instruments on board the WIND spacecraft are used to study statistically the structure of the front of oblique interplanetary shock waves
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::39616a8ea46e19ee377f8a9f5af078db
https://doi.org/10.1134/s001679321806004x
https://doi.org/10.1134/s001679321806004x
Autor:
Sergey Khomutov, Aleksandr Yahnin, Raita Tero, B. Tsegmed, Vladimir Parhomov, Vitaliy Chilikin, Aleksandr Pashinin, N. L. Borodkova, Aleksey Mochalov
Publikováno v:
Solar-Terrestrial Physics, Vol 4, Iss 3, Pp 52-66 (2018)
Using the June 22, 2015 event as an example, we present new data confirming the presence of a precursor of the sudden magnetic impulse caused by a powerful interplanetary shock wave (ISW). The precursor in the form of a train of oscillations (broadba
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4482cc362e0b31dd95ee459b2c46f792
https://doi.org/10.12737/szf-43201808
https://doi.org/10.12737/szf-43201808
Autor:
Vitaliy Chilikin, Maxim Eselevich, N. L. Borodkova, Vladimir Parhomov, Aleksey Dmitriev, Viktor Eselevich
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 4, Pp 44-57 (2017)
In Earth’s orbit on June 28, 1999, there was a diamagnetic structure (DS) representing a filament with a uniquely high speed (about 900 km/s). We show that the filament is a part of the specific sporadic solar wind (SW) stream, which is characteriz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b12f83d97dd4c8cdb0c3598681141b0
https://doi.org/10.12737/szf-34201705
https://doi.org/10.12737/szf-34201705