Zobrazeno 1 - 10
of 43
pro vyhledávání: '"A. Y. Ukhorskiy"'
Autor:
K. A. Sorathia, M. Shumko, A. Sciola, A. Michael, V. G. Merkin, B. Gallardo‐Lacourt, M. G. Henderson, D. Lin, S. Bao, J. Garretson, A. Y. Ukhorskiy
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 16, Pp n/a-n/a (2024)
Abstract We present the first global geospace simulation to reproduce auroral giant undulations (GUs). To identify their magnetospheric drivers, we employ the MAGE (Multiscale Atmosphere‐Geospace Environment) model in a case study of a geomagnetic
Externí odkaz:
https://doaj.org/article/edc1fff38b3844b8a70a640d51ba49bc
Autor:
A. Briard, J.-F. Ripoll, A. Michael, B.-J. Gréa, G. Peyrichon, M. Cosmides, H. El-Rabii, M. Faganello, V. G. Merkin, K. A. Sorathia, A. Y. Ukhorskiy, J. G. Lyon, A. Retino, V. Bouffetier, L. Ceurvorst, H. Sio, O. A. Hurricane, V. A. Smalyuk, A. Casner
Publikováno v:
Frontiers in Physics, Vol 12 (2024)
Introduction: The Kelvin–Helmholtz Instability (KHI) is an interface instability that develops between two fluids or plasmas flowing with a common shear layer. KHI occurs in astrophysical jets, solar atmosphere, solar flows, cometary tails, planeta
Externí odkaz:
https://doaj.org/article/48184d4c20cd4ae391b8c0960d70bb39
Autor:
J.-F. Ripoll, V. Pierrard, G. S. Cunningham, X. Chu, K. A. Sorathia, D. P. Hartley, S. A. Thaller, V. G. Merkin, G. L. Delzanno, S. De Pascuale, A. Y. Ukhorskiy
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
This review focusses strictly on existing plasma density models, including ionospheric source models, empirical density models, physics-based and machine-learning density models. This review is framed in the context of radiation belt physics and spac
Externí odkaz:
https://doaj.org/article/9e27abf551b44719b7dfb163e6e73416
Publikováno v:
Annales Geophysicae, Vol 27, Pp 2173-2181 (2009)
During geomagnetic storms relativistic electron fluxes in the outer radiation belt exhibit dynamic variability over multiple orders of magnitude. This requires radial transport of electrons across their drift shells and implies violation of their
Externí odkaz:
https://doaj.org/article/9cd603598e1549ef8cfd0347f0076f44
Publikováno v:
Annales Geophysicae, Vol 21, Pp 1913-1929 (2003)
The solar wind-magnetosphere coupling during substorms exhibits dynamical features in a wide range of spatial and temporal scales. The goal of our work is to combine the global and multi-scale description of magnetospheric dynamics in a unified
Externí odkaz:
https://doaj.org/article/ddc65083cf694534a31fdddef39b2a8d
Autor:
Simon Wing, Drew L. Turner, Aleksandr Y. Ukhorskiy, Jay R. Johnson, Thomas Sotirelis, Romina Nikoukar, Giuseppe Romeo
Publikováno v:
Space Weather. 20
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Autor:
Aleksandr Y, Ukhorskiy, Kareem A, Sorathia, Viacheslav G, Merkin, Chris, Crabtree, Alex C, Fletcher, David M, Malaspina, Steven J, Schwartz
Publikováno v:
Scientific Reports. 12
Plasma convection in the Earth’s magnetosphere from the distant magnetotail to the inner magnetosphere occurs largely in the form of mesoscale flows, i.e., discrete enhancements in the plasma flow with sharp dipolarizations of magnetic field. Recen
Autor:
Kazue Takahashi, Chris Crabtree, A. Y. Ukhorskiy, Alexander Boyd, Richard E. Denton, Drew Turner, Matina Gkioulidou, Massimo Vellante, Harlan E. Spence
Previous spacecraft studies showed that stormtime poloidal ultralow-frequency (ULF) waves in the ring current region have an antisymmetric (second harmonic) mode structure about the magnetic equator. This paper reports Van Allen Probes observations o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db4cc72f31cb90be8e167fbbb678e91c
http://hdl.handle.net/11697/181372
http://hdl.handle.net/11697/181372
An empirical model of radiation belt relativistic electrons (m = 560–875 MeV G–1 and I = 0.088–0.14 RE G0.5) with average energy ~ 1.3 MeV is developed. The model i...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::274dd0118b0a8177fcf5f419b14bb068
https://doi.org/10.1002/essoar.10508583.1
https://doi.org/10.1002/essoar.10508583.1