Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Runov Andrei"'
Autor:
Wilkins, Colin, Angelopoulos, Vassilis, Artemyev, Anton, Runov, Andrei, Zhang, Xiao-Jia, Liu, Jiang, Tsai, Ethan
Using particle data from the ELFIN satellites, we present a statistical study of 284 proton isotropy boundary events on the nightside magnetosphere, characterizing their occurrence and distribution in local time, latitude (L-shell), energy, and preci
Externí odkaz:
http://arxiv.org/abs/2409.04488
Autor:
Zhang, Xiao-Jia, Artemyev, Anton V., Li, Xinlin, Arnold, Harry, Angelopoulos, Vassilis, Turner, Drew L., Shumko, Mykhaylo, Runov, Andrei, Mei, Yang, Xiang, Zheng
Earth's magnetotail, a night-side region characterized by stretched magnetic field lines and strong plasma currents, is the primary site for the release of magnetic field energy and its transformation into plasma heating and kinetic energy plus charg
Externí odkaz:
http://arxiv.org/abs/2408.17299
Autor:
Wilkins, Colin, Angelopoulos, Vassilis, Runov, Andrei, Artemyev, Anton, Zhang, Xiao-Jia, Liu, Jiang, Tsai, Ethan
Utilizing observations from the ELFIN satellites, we present a statistical study of $\sim$2000 events in 2019-2020 characterizing the occurrence in magnetic local time (MLT) and latitude of $\geq$50 keV electron isotropy boundaries (IBs) at Earth, an
Externí odkaz:
http://arxiv.org/abs/2305.16260
Publikováno v:
ApJ 952 (2023) 36
Force-free current sheets are local plasma structures with field-aligned electric currents and approximately uniform plasma pressures. Such structures, widely found throughout the heliosphere, are sites for plasma instabilities and magnetic reconnect
Externí odkaz:
http://arxiv.org/abs/2301.04590
Autor:
Barbhuiya, M. Hasan, Cassak, Paul. A., Shay, Michael. A., Roytershteyn, Vadim, Swisdak, Marc, Caspi, Amir, Runov, Andrei, Liang, Haoming
Publikováno v:
Journal of Geophysical Research: Space Physics, Vol. 127, Issue 8, e2022JA030610 (22pp); 2022 August 08
Electron ring velocity space distributions have previously been seen in numerical simulations of magnetic reconnection exhausts and have been suggested to be caused by the magnetization of the electron outflow jet by the compressed reconnected magnet
Externí odkaz:
http://arxiv.org/abs/2208.00559
Autor:
Artemyev, Anton, Reville, Victor, Zimovets, Ivan, Nishimura, Yukitoshi, Velli, Marco, Runov, Andrei, Angelopoulos, Vassilis
Magnetic field line reconnection is a universal plasma process responsible for the magnetic field topology change and magnetic field energy dissipation into charged particle heating and acceleration. In many systems, the conditions leading to the mag
Externí odkaz:
http://arxiv.org/abs/2205.01935
Publikováno v:
Geophysical Research Letters, 49, e2022GL097870 (2022)
The magnetotail current sheet configuration determines magnetic reconnection properties that control the substorm onset, one of the most energetic phenomena in the Earth's magnetosphere. The quiet-time current sheet is often approximated as a two-dim
Externí odkaz:
http://arxiv.org/abs/2202.09539
Publikováno v:
Physics of Plasmas 29, 092901 (2022)
Many in-situ spacecraft observations have demonstrated that magnetic reconnection in the Earth's magnetotail is largely controlled by the pre-reconnection current sheet configuration. One of the most important thin current sheet characteristics is th
Externí odkaz:
http://arxiv.org/abs/2202.06204
Autor:
Artemyev, Anton, Zimovets, Ivan, Sharykin, Ivan, Nishimura, Yukitoshi, Downs, Cooper, Weygand, James, Fiori, Robyn, Zhang, Xiao-Jia, Runov, Andrei, Velli, Marco, Angelopoulos, Vassilis, Panasenco, Olga, Russell, Christopher, Miyoshi, Yoshizumi, Kasahara, Satoshi, Matsuoka, Ayako, Yokota, Shoichiro, Keika, Kunihiro, Hori, Tomoaki, Kazama, Yoichi, Wang, Shiang-Yu, Shinohara, Iku, Ogawa, Yasunobu
Magnetic field-line reconnection is a universal plasma process responsible for the conversion of magnetic field energy to the plasma heating and charged particle acceleration. Solar flares and Earth's magnetospheric substorms are two most investigate
Externí odkaz:
http://arxiv.org/abs/2105.03772
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