Zobrazeno 1 - 10
of 17
pro vyhledávání: '"M. V. Kubyshkina"'
Autor:
D. B. Korovinskiy, D. I. Kubyshkina, V. S. Semenov, M. V. Kubyshkina, N. V. Erkaev, S. A. Kiehas
Publikováno v:
Annales Geophysicae, Vol 36, Pp 641-653 (2018)
A specific class of solutions of the Vlasov–Maxwell equations, developed by means of generalization of the well-known Harris–Fadeev–Kan–Manankova family of exact two-dimensional equilibria, is studied. The examined model reproduces the curre
Externí odkaz:
https://doaj.org/article/cf2839a75e964ebf9ee91a059a15f43e
Publikováno v:
Geoscience Letters, Vol 4, Iss 1, Pp 1-7 (2017)
Abstract The time scales of reconnection outflow, substorm expansion, and development of instabilities in the terrestrial magnetosphere are comparable, i.e., from several to tens of minutes, and their existence is related. In this paper, we investiga
Externí odkaz:
https://doaj.org/article/d83e828bccd246beb3c3f8c58ffd8006
Autor:
A. V. Nikolaev, V. A. Sergeev, N. A. Tsyganenko, M. V. Kubyshkina, H. Opgenoorth, H. Singer, V. Angelopoulos
Publikováno v:
Annales Geophysicae, Vol 33, Pp 505-517 (2015)
Substorm current wedge (SCW) formation is associated with global magnetic field reconfiguration during substorm expansion. We combine a two-loop model SCW (SCW2L) with a background magnetic field model to investigate distortion of the ionospheric
Externí odkaz:
https://doaj.org/article/f7db4a876a004f2d89ab2a57f172b5ab
Autor:
J. R. Kan, H. Li, C. Wang, H. U. Frey, M. V. Kubyshkina, A. Runov, C. J. Xiao, L. H. Lyu, W. Sun
Publikováno v:
Annales Geophysicae, Vol 29, Pp 2045-2059 (2011)
We present a new M-I coupling model of substorm during southward IMF based on the THEMIS observations of two events on 1 March 2008. The first event (E-1) was classified as a pseudo-breakup: brightening of the onset arc preceded the first dipolari
Externí odkaz:
https://doaj.org/article/f30f4f3382c14d61b9a207ca365212ad
Publikováno v:
Annales Geophysicae, Vol 27, Pp 417-425 (2009)
One-fluid ideal MHD model is applied for description of current sheet flapping disturbances appearing due to a gradient of the normal magnetic field component. The wave modes are studied which are associated to the flapping waves observed in the
Externí odkaz:
https://doaj.org/article/4ad40631c7b944e9a3ac450414dc2063
Autor:
S. V. Apatenkov, V. A. Sergeev, M. V. Kubyshkina, R. Nakamura, W. Baumjohann, A. Runov, I. Alexeev, A. Fazakerley, H. Frey, S. Muhlbachler, P. W. Daly, J.-A. Sauvaud, N. Ganushkina, T. Pulkkinen, G. D. Reeves, Y. Khotyaintsev
Publikováno v:
Annales Geophysicae, Vol 25, Pp 801-814 (2007)
Addressing the origin of the energetic particle injections into the inner magnetosphere, we investigate the 23 February 2004 substorm using a favorable constellation of four Cluster (near perigee), LANL and Geotail spacecraft. Both an energy-dispe
Externí odkaz:
https://doaj.org/article/bd1043c3d0474bcb9cda5b8d4401999f
Autor:
V. A. Sergeev, M. V. Kubyshkina, W. Baumjohann, R. Nakamura, O. Amm, T. Pulkkinen, V. Angelopoulos, S. B. Mende, B. Klecker, T. Nagai, J.-A. Sauvaud, J. A. Slavin, M. F. Thomsen
Publikováno v:
Annales Geophysicae, Vol 23, Pp 2183-2198 (2005)
Transition from the growth phase to the substorm expansion during a well-isolated substorm with a strong growth phase is investigated using a unique radial (THEMIS-like) spacecraft constellation near midnight, including the probing of the tail cur
Externí odkaz:
https://doaj.org/article/835ef12867f842b99312b4718cfba9fa
Autor:
N. Yu. Ganushkina, T. I. Pulkkinen, M. V. Kubyshkina, V. A. Sergeev, E. A. Lvova, T. A. Yahnina, A. G. Yahnin, T. Fritz
Publikováno v:
Annales Geophysicae, Vol 23, Pp 1839-1847 (2005)
Polar CAMMICE MICS proton pitch angle distributions with energies of 31-80 keV were analyzed to determine the locations where anisotropic pitch angle distributions (perpendicular flux dominating) change to isotropic distributions. We compared the
Externí odkaz:
https://doaj.org/article/73d0b403e4c34d5cb45e0130e2962563
Autor:
V. V. Kalegaev, N. Y. Ganushkina, T. I. Pulkkinen, M. V. Kubyshkina, H. J. Singer, C. T. Russell
Publikováno v:
Annales Geophysicae, Vol 23, Pp 523-533 (2005)
We study the dynamics of the magnetospheric large-scale current systems during storms by using three different magnetospheric magnetic field models: the paraboloid, event-oriented, and Tsyganenko T01 models. We have modelled two storm events, one
Externí odkaz:
https://doaj.org/article/bfb8773874a64c89b4bedb3391fe6cdc
Publikováno v:
Annales Geophysicae, Vol 22, Pp 1317-1334 (2004)
We present a method to model the storm-time magnetospheric magnetic field using representations of the magnetic field arising from the various magnetospheric current systems. We incorporate the effects of magnetotail changes during substorms by in
Externí odkaz:
https://doaj.org/article/e240995b361b468aa7057a141a50720f