Zobrazeno 1 - 10
of 346
pro vyhledávání: '"A. V Artemyev"'
Autor:
Jing‐Huan Li, Xu‐Zhi Zhou, Shan Wang, Zhi‐Yang Liu, Qiu‐Gang Zong, Shu‐Tao Yao, Anton V. Artemyev, Yoshiharu Omura, Li Li, Chao Yue, Quan‐Qi Shi
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 20, Pp n/a-n/a (2024)
Abstract The terrestrial bow shock is the boundary where supersonic solar wind slows down abruptly near the magnetopause. The shock front geometry could be modulated by surface waves to form rippled structures, which impact the acceleration process o
Externí odkaz:
https://doaj.org/article/f6a863651d74427ab01276c139de1808
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 17, Pp n/a-n/a (2024)
Abstract Night‐side chorus waves are often observed during plasma sheet injections, typically confined around the equator and thus potentially responsible for precipitation of ≲100 keV electrons. However, recent low‐altitude observations have r
Externí odkaz:
https://doaj.org/article/a87a855fc0894efba79f12d2e359dab0
Autor:
Sergey A. Simonov, Alexander V. Artemyev, Nikolay V. Lapshin, Andrey O. Tolstoguzov, Maria V. Matantseva
Publikováno v:
Nature Conservation Research: Заповедная наука, Vol 9, Iss 1, Pp 30-44 (2024)
Olonets grasslands (61.041111° N, 32.931389° E) are the most extensive agrolandscapes in the Republic of Karelia (Northwest Russia), one of the largest spring stopovers of migrating birds in Northern Europe and a breeding area of farmland-associate
Externí odkaz:
https://doaj.org/article/1cb0ea9b9b5542f4af1319dca22d8dd4
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 14, Pp n/a-n/a (2024)
Abstract Energetic electron precipitation (EEP) during substorms significantly affects ionospheric chemistry and lower‐ionosphere (
Externí odkaz:
https://doaj.org/article/13334a5a6c9346358563f5317d00c8c5
Autor:
Veronika S. Grach, Anton V. Artemyev, Andrei G. Demekhov, Xiao‐Jia Zhang, Jacob Bortnik, Vassilis Angelopoulos
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 9, Pp n/a-n/a (2024)
Abstract Electromagnetic ion cyclotron (EMIC) waves can very rapidly and effectively scatter relativistic electrons into the atmosphere. EMIC‐driven precipitation bursts can be detected by low‐altitude spacecraft, and analysis of the fine structu
Externí odkaz:
https://doaj.org/article/770bf3a4ba0945fa92d85ffdd45e4b35
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 4, Pp n/a-n/a (2024)
Abstract Sub‐auroral polarization streams (SAPS) are one of the most intense manifestations of magnetosphere‐ionosphere coupling. Magnetospheric energy transport to the ionosphere within SAPS is associated with Poynting flux and the precipitation
Externí odkaz:
https://doaj.org/article/1c90082eb19741878768c7a3b20ca073
Autor:
I. Y. Vasko, F. S. Mozer, T. Bowen, J. Verniero, X. An, A. V. Artemyev, S. D. Bale, J. W. Bonnell, J. Halekas, I. V. Kuzichev
Publikováno v:
The Astrophysical Journal Letters, Vol 967, Iss 2, p L31 (2024)
Parker Solar Probe measurements have recently shown that coherent fast magnetosonic and Alfvén ion-cyclotron waves are abundant in the solar wind and can be accompanied by higher-frequency electrostatic fluctuations. In this Letter we reveal the non
Externí odkaz:
https://doaj.org/article/1daf1866b9a6446d904cb4cca0531a95
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
Resonant interactions with whistler-mode waves are a crucial mechanism that drives the precipitation of energetic electrons. Using test particle simulations, we investigated the impact of nonlinear interactions of whistler-mode waves on electron prec
Externí odkaz:
https://doaj.org/article/d78b9a21dbc74a7083a835f723abdcca
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 21, Pp n/a-n/a (2023)
Abstract Energetic electron precipitation from the equatorial magnetosphere into the atmosphere plays an important role in magnetosphere‐ionosphere coupling: precipitating electrons alter ionospheric properties, whereas ionospheric outflows modify
Externí odkaz:
https://doaj.org/article/484b0d9e80744d49b9511197cbf079b0
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.