Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Daniil Korovinskiy"'
Autor:
Andrey Divin, Ildar Shaikhislamov, Igor Paramonik, Marina Rumenskikh, Daniil Korovinskiy, Jan Deca
Magnetospheres are formed when plasma flow interacts with an external source of the magnetic field. Objects (with a size comparable to or less than the ion inertial length or ion gyroradius) formed by relatively weak magnetic field sources are called
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8d5fffcbcd2b86fa04e640a7d82d6fa6
https://doi.org/10.5194/egusphere-egu22-12904
https://doi.org/10.5194/egusphere-egu22-12904
The compressible electron magnetohydrodynamics (EMHD) Grad–Shafranov (GS) reconstruction technique is applied to recover a magnetic reconnection electron diffusion region (EDR) immersed in a flux‐rope type dipolarization front observed by the Mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f25cafa64193abce94c114701ccb6d0
https://doi.org/10.5194/egusphere-egu22-4579
https://doi.org/10.5194/egusphere-egu22-4579
Autor:
Martin Hosner, Rumi Nakamura, Daniel Schmid, Takuma Nakamura, Evgeny Panov, Daniil Korovinskiy
The Dipolarization Front (DF), which is a sharp increase of the northward magnetic field component, accompanied by fast earthward-moving plasma flows, is a well known phenomenon in the Earth's Magnetotail. Plasma characteristics also change at the fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3025fe02a9400221ca02b7aabec21082
https://doi.org/10.5194/egusphere-egu22-5853
https://doi.org/10.5194/egusphere-egu22-5853
Autor:
I. V. Kubyshkin, E. V. Panov, Andrey Divin, S. A. Kiehas, Vladimir Semenov, Daniil Korovinskiy, Nikolai V. Erkaev
Publikováno v:
Journal of Geophysical Research: Space Physics. 126
Autor:
Marina Rumenskikh, Ivan Zaitsev, Ildar Shaikhislamov, Andrey Divin, Jan Deca, Vladimir Semenov, Daniil Korovinskiy
In this study, we use a combination of 3D Particle-in-Cell (PIC) simulations and a laboratory experiment to investigate the dynamics of solar wind - Moon interaction. It is known that the Moon has no global magnetic field, but there exist areas of in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::96548aa9063ad91e6c6dbdf50bbe8bc9
https://doi.org/10.5194/egusphere-egu21-16209
https://doi.org/10.5194/egusphere-egu21-16209
Autor:
Andrey Divin, Daniil Korovinskiy, Vladimir Semenov, Ivan Zaitsev, Stefano Markidis, Yuri V. Khotyaintsev, Jan Deca
Various simulations of collisionless magnetic reconnection reveal that the process is typically fast, with the reconnection rate being of the order of 0.1. Systematic numerical and observational studies of upstream parameters dependence (density, mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b292b369e8f5cdd6aeed5741bf592502
https://doi.org/10.5194/egusphere-egu21-13267
https://doi.org/10.5194/egusphere-egu21-13267
We perform a five year statistical study of fast flows in the Earth's magnetotail observed by ARTEMIS to investigate their occurrence rate, dawn-dusk asymmetry and relation with magnetospheric substorms. Almost half of the observed flows are directed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3acd8b4d9bd6523c0fdf11601d37704c
https://doi.org/10.5194/egusphere-egu2020-11901
https://doi.org/10.5194/egusphere-egu2020-11901
The problem of steady symmetrical two-dimensional magnetic reconnection is addressed in terms of the EMHD approximation. In the immediate vicinity of the X-point, this approach has been proven to be an appropriate frame for the reconstruction problem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ffd71f67d7d0b7f3b81a18cfd1458d4e
https://doi.org/10.5194/egusphere-egu2020-8673
https://doi.org/10.5194/egusphere-egu2020-8673
Autor:
Andrey Divin, Jan Deca, Stefano Markidis, Daniil Korovinskiy, Giovanni Lapenta, Ivan Zaitsev, Viacheslav Olshevsky, Vladimir Semenov
We study inflow density dependence of substructures within electron diffusion region (EDR) of collisionless symmetric magnetic reconnection. We perform a set of 2.5D particle-in-cell simulations which start from a Harris current layer with a uniform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06aaf1e75fd5415baa2a2ab8bbf84239
https://lirias.kuleuven.be/handle/123456789/642691
https://lirias.kuleuven.be/handle/123456789/642691