Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Tenishev Valeriy"'
Autor:
Huang, Zhenguang, Toth, Gabor, Gombosi, Tamas I., Combi, Michael R., Jia, Xianzhe, Shou, Yinsi, Tenishev, Valeriy, Altwegg, Kathrin, Rubin, Martin
The interaction between a Coronal Mass Ejection (CME) and a comet has been observed several times by in-situ observations from the Rosetta Plasma Consortium (RPC), which is designed to investigate the cometary magnetosphere of comet 67P/Churyumov-Ger
Externí odkaz:
http://arxiv.org/abs/2403.05779
Autor:
Gombosi Tamas I., Chen Yuxi, Glocer Alex, Huang Zhenguang, Jia Xianzhe, Liemohn Michael W., Manchester Ward B., Pulkkinen Tuija, Sachdeva Nishtha, Al Shidi Qusai, Sokolov Igor V., Szente Judit, Tenishev Valeriy, Toth Gabor, van der Holst Bart, Welling Daniel T., Zhao Lulu, Zou Shasha
Publikováno v:
Journal of Space Weather and Space Climate, Vol 11, p 42 (2021)
Magnetohydrodynamics (MHD)-based global space weather models have mostly been developed and maintained at academic institutions. While the “free spirit” approach of academia enables the rapid emergence and testing of new ideas and methods, the la
Externí odkaz:
https://doaj.org/article/317f30891d9f4187952d9546e2493282
Deriving properties of cometary nuclei from coma data is of significant importance for our understanding of cometary activity and has implications beyond. Ground-based data represent the bulk of measurements available for comets. Yet, to date these o
Externí odkaz:
http://arxiv.org/abs/2308.05797
Autor:
Tenishev, Valeriy1 (AUTHOR) valeriy.m.tenishev@nasa.gov, Shou, Yinsi2 (AUTHOR), Lee, Yuni3,4 (AUTHOR), Ma, Yingjuan5 (AUTHOR), Combi, Michael R.2 (AUTHOR)
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p1-23. 23p.
The need for quantitative characterization of the solar energetic particle (SEP) dynamics goes beyond being an academic discipline only. It has numerous practical implications related to human activity in space. The terrestrial magnetic field shields
Externí odkaz:
http://arxiv.org/abs/2209.09346
Exoplanets orbiting M-dwarfs within habitable zones are exposed to stellar environments more extreme than that terrestrial planets experience in our Solar System, which can significantly impact the atmospheres of the exoplanets and affect their habit
Externí odkaz:
http://arxiv.org/abs/2109.06963
Space plasma simulations have seen an increase in the use of magnetohydrodynamic (MHD) with embedded Particle-in-Cell (PIC) models. This combined MHD-EPIC algorithm simulates some regions of interest using the kinetic PIC method while employing the M
Externí odkaz:
http://arxiv.org/abs/2108.05425
Neutral hydrogen has been shown to greatly impact the plasma flow in the heliopshere and the location of the heliospheric boundaries. We present the results of the Solar-wind with Hydrogen Ion Exchange and Large-scale Dynamics (SHIELD) model, a new,
Externí odkaz:
http://arxiv.org/abs/2004.01152
Autor:
Zheng, Yihua, Jun, Insoo, Tu, Weichao, Shprits, Yuri Y., Kim, Wousik, Matthiä, Daniel, Meier, Matthias M., Kent Tobiska, W., Miyoshi, Yoshizumi, Jordanova, Vania K., Ganushkina, Natalia Y., Tenishev, Valeriy, O’Brien, T.P., Brunet, Antoine, Maget, Vincent, Guo, Jingnan, Wang, Dedong, Horne, Richard B., Glauert, Sarah, Haas, Bernhard, Drozdov, Alexander Y.
Publikováno v:
In Advances in Space Research May 2024
Autor:
Sokolov, Igor V., Sun, Haomin, Toth, Gabor, Huang, Zhenguang, Tenishev, Valeriy, Zhao, Lulu, Kota, Jozsef, Cohen, Ofer, Gombosi, Tamas
Simulation of plasmas in electromagnetic fields requires numerical solution of a kinetic equation that describes the time evolution of the particle distribution function. In this paper we propose a finite volume scheme based on integral relation for
Externí odkaz:
http://arxiv.org/abs/1910.12636