Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Ilya Kuzichev"'
With the increased availability of ground magnetic field measurements from the Northern and Southern hemispheres at higher latitudes, further insight could be gained into how the physical processes coupling magnetosphere and ionosphere vary with sola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac7cb194bbc641a5c3993113d14ff47c
https://doi.org/10.5194/egusphere-egu23-7628
https://doi.org/10.5194/egusphere-egu23-7628
Autor:
Ilya Kuzichev, Ivan Vasko
Whistler waves play important role in electron dynamics in space plasmas. They are capable of accelerating and scattering electrons, shaping the electron velocity distribution function of the solar wind electrons and providing a mechanism to fill the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::810a1bbfb3d9fbc4d1fba61e65461d9d
https://doi.org/10.5194/egusphere-egu23-11923
https://doi.org/10.5194/egusphere-egu23-11923
Autor:
Sung‐Jun Noh, Hyomin Kim, Marc Lessard, Mark Engebretson, Vyacheslav Pilipenko, Eun‐Hwa Kim, Jay Johnson, Ilya Kuzichev, Michelle Salzano
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Autor:
Ilya Kuzichev, A. R. Soto-chavez
Whistler-mode chorus waves are one of the most intense wave phenomena in the Earth’s inner magnetosphere. They are considered to be a major driver of the outer radiation belt dynamics, as they can efficiently scatter and energize electrons via reso
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::442a67bb32166841d8c932ff4dea409a
https://doi.org/10.5194/egusphere-egu21-14307
https://doi.org/10.5194/egusphere-egu21-14307
The electron heat flux is one of the leading terms in energy flow processes in the collisionless or weakly-collisional solar wind plasma. The very first observations demonstrated that the collisional Spitzer-HÓrm law could not describe the heat fl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::703e8a2cec5ea715ba69b706b5bd7e96
https://doi.org/10.5194/egusphere-egu2020-1175
https://doi.org/10.5194/egusphere-egu2020-1175
Electron holes are nonlinear electrostatic structures that are often observed in the vicinity of the magnetotail energy release regions, e.g. magnetic reconnection. In this work we develop 1.5D Vlasov code simulations of the electron hole dynamics in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::650b557dd842db41988e926cb5bbd375
https://doi.org/10.5194/egusphere-egu2020-11967
https://doi.org/10.5194/egusphere-egu2020-11967
Publikováno v:
Geophysical Research Letters. 44:2105-2112
Electron phase space holes (EH) are electrostatic solitary waves that are widely observed in the space plasma often permeated by inhomogeneous magnetic fields. Understanding of the EH evolution in inhomogeneous magnetic fields is critical for accurat
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:120-135