Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Talgat Manglayev"'
Autor:
Talgat Manglayev, Refik Caglar Kizilirmak, Yau Hee Kho, Nor Asilah Wati Abdul Hamid, Yue Tian
Publikováno v:
Wireless Personal Communications. 124:3253-3261
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2822759f28e59ebaf77a412605675061
https://doi.org/10.1007/s11277-022-09511-6
https://doi.org/10.1007/s11277-022-09511-6
Autor:
Maxime Grandin, Thijs Luttikhuis, Markku Alho, Markus Battarbee, Maarja Bussov, Giulia Cozzani, Maxime Dubart, Urs Ganse, Harriet George, Konstantinos Horaites, Talgat Manglayev, Konstantinos Papadakis, Yann Pfau-Kempf, Jonas Suni, Vertti Tarvus, Lucile Turc, Ivan Zaitsev, Hongyang Zhou, Minna Palmroth
The precipitation of charged particles from the magnetosphere into the ionosphere is one of the crucial coupling mechanisms between these two regions of geospace. While precipitating particle fluxes have been measured by numerous spacecraft missions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b092ad5b6b096cf8e43b077cc295f22
https://doi.org/10.5194/egusphere-egu22-7611
https://doi.org/10.5194/egusphere-egu22-7611
Autor:
Giulia Cozzani, Urs Ganse, Yann Pfau-Kempf, Markku Alho, Jonas Suni, Maxime Grandin, Lucile Turc, Ivan Zaitsev, Maarja Bussov, Maxime Dubart, Harriet George, Konstantinos Horaites, Talgat Manglayev, Konstantinos Papadakis, Vertti Tarvus, Honyang Zhou, Minna Palmroth
Magnetic reconnection is a fundamental process in plasma and a major cause of energy conversion and transport by means of magnetic field topology reconfiguration. It takes place in thin plasma sheets, where energy is often explosively converted from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::07aa4588f0fb23b7e90d00dde3d4f2a2
https://doi.org/10.5194/egusphere-egu22-7069
https://doi.org/10.5194/egusphere-egu22-7069
Autor:
Vertti Tarvus, Lucile Turc, Hongyang Zhou, Giulia Cozzani, Urs Ganse, Yann Pfau-Kempf, Markku Alho, Markus Battarbee, Maarja Bussov, Maxime Dubart, Harriet George, Maxime Grandin, Konstantinos Horaites, Talgat Manglayev, Konstantinos Papadakis, Jonas Suni, Ivan Zaitsev, Minna Palmroth
The Kelvin-Helmholtz instability (KHI) is a ubiquitous fluid instability in space plasmas. At the flanks of Earth's magnetopause, the KHI can typically develop during periods of northward interplanetary magnetic field, and it drives the solar wind-ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1c17a65b86bba24b1afd823be0433b51
https://doi.org/10.5194/egusphere-egu22-7354
https://doi.org/10.5194/egusphere-egu22-7354
Autor:
Ivan Zaitsev, Andrey Divin, Urs Ganse, Yann Pfau-Kempf, Markus Battarbee, Markku Alho, Jonas Suni, Maxime Grandin, Lucile Turc, Giulia Cozzani, Maarja Bussov, Maxime Dubart, Harriet George, Konstantinos Horaites, Konstantinos Papadakis, Talgat Manglayev, Vertti Tarvus, Honyang Zhou, Minna Palmroth
Magnetic reconnection is the energy converter in space plasma that releases magnetic energy into the kinetic energy of particles. We study the magnetotail reconnection in the first 3D global magnetospheric hybrid-Vlasov simulation performed with Vlas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8a43a363d1fc0fd0ba7c51c5b6edac9
https://doi.org/10.5194/egusphere-egu22-6378
https://doi.org/10.5194/egusphere-egu22-6378
Autor:
Maxime Dubart, Markus Battarbee, Urs Ganse, Felix Spanier, Jonas Suni, Andreas Johlander, Markku Alho, Maarja Bussov, Giulia Cozzani, Harriet George, Maxime Grandin, Talgat Manglayev, Kostis Papadakis, Yann Pfau-Kempf, Vertti Tarvus, Lucile Turc, Ivan Zaitsev, Hongyang Zhou, Minna Palmroth
Numerical simulations play a central role in modern sciences. The trade-off between the accuracy of the physical processes described and the cost of computational resources is often the main limiting factor in these simulations. In global hybrid-Vlas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4170431d69b7e8f0e5cf301868085aec
https://doi.org/10.5194/egusphere-egu22-3429
https://doi.org/10.5194/egusphere-egu22-3429
Autor:
Konstantinos Horaites, Markku Alho, Markus Battarbee, Maxime Dubart, Urs Ganse, Harriet George, Maxime Grandin, Talgat Manglayev, Minna Palmroth, Konstantinos Papadakis, Jonas Suni, Vertti Tarvus, Lucile Turc, Ivan Zaitsev, Hongyang Zhou
Vlasiator (https://www2.helsinki.fi/en/researchgroups/vlasiator) is a high-performance kinetic code that is now conducting the first ever 3D hybrid-Vlasov simulations of the global magnetospheric system. In recent months, the driving conditions of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c06bf863bf3f1643260ee05916711361
https://doi.org/10.5194/egusphere-egu22-4687
https://doi.org/10.5194/egusphere-egu22-4687
Autor:
Hongyang Zhou, Lucile Turc, Vertti Tarvus, Yann Pfau-Kempf, Markus Battarbee, Maxime Dubart, Urs Ganse, Markku Alho, Maxime Grandin, Harriet George, Jonas Suni, Maarja Bussov, Konstantinos Papadakis, Talgat Manglayev, Kosta Horaites, Ivan Zaitsev, Giulia Cozzani, Minna Palmroth
Ultra-low frequency (ULF) waves in the Pc5 range, with periods between 150 – 600 s, play a key role in the dynamics of Earth’s magnetosphere, in particular through their interaction with radiation belt electrons. One important source of magnetosp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f3955f78554b0a79a561d397082f2352
https://doi.org/10.5194/egusphere-egu22-5653
https://doi.org/10.5194/egusphere-egu22-5653
Autor:
Minna Palmroth, Urs Ganse, Yann Pfau-Kempf, Markku Alho, Jonas Suni, Maxime Grandin, Lucile Turc, Markus Battarbee, Andreas Johlander, Vertti Tarvus, Hongyang Zhou, Maarja Bussov, Maxime Dubart, Harriet George, Konstantinos Horaites, Talgat Manglayev, Konstantinos Papadakis, Rumi Nakamura, Tuija Pulkkinen
Among the most unpredictable phenomena within the near-Earth space are substorms, periods of energy loading and explosive release within the magnetospheric tail. Substorms are global, as energy is extracted from the solar wind via dayside reconnectio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::df4f012bac494a3268775d28250bacbb
https://doi.org/10.5194/egusphere-egu22-3573
https://doi.org/10.5194/egusphere-egu22-3573
Publikováno v:
Wireless Personal Communications. 103:2391-2400
Non-orthogonal multiple access (NOMA) can achieve high throughput by using the same time and frequency resources for multiple users. NOMA distinguishes multiple users in power domain by computationally-heavy successive interference cancellation (SIC)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aa196b00dbaa99a0cc510bad91457518
https://doi.org/10.1007/s11277-018-5915-y
https://doi.org/10.1007/s11277-018-5915-y