Zobrazeno 1 - 10
of 1 211
pro vyhledávání: '"Tóth, Gabor"'
Autor:
Liu, Weihao, Sokolov, Igor V., Zhao, Lulu, Gombosi, Tamas I., Chen, Xiaohang, Sachdeva, Nishtha, Tóth, Gábor, Manchester IV, Ward B., Lario, David, Whitman, Kathryn, Bruno, Alessandro, Cohen, Christina M. S., Mays, M. Leila, Bain, Hazel M.
Solar energetic particles (SEPs) can pose hazardous radiation risks to both humans in space and spacecraft electronics. Numerical modeling based on first principles offers valuable insights into SEPs, providing synthetic observables for SEPs at any t
Externí odkaz:
http://arxiv.org/abs/2412.07581
Autor:
Shay, Michael, Adhikari, Subash, Beesho, Naoki, Birn, Joachim, Buechner, Jorg, Cassak, Paul, Chen, Li-Jen, Chen, Yuxi, Cozzani, Giulia, Drake, Jim, Guo, Fan, Hesse, Michael, Jain, Neeraj, Pfau-Kempf, Yann, Lin, Yu, Liu, Yi-Hsin, Oka, Mitsuo, Omelchenko, Yuri A., Palmroth, Minna, Pezzi, Oreste, Reiff, Patricia H., Swisdak, Marc, Toffoletto, Frank, Toth, Gabor, Wolf, Richard A.
Simulations have played a critical role in the advancement of our knowledge of magnetic reconnection. However, due to the inherently multiscale nature of reconnection, it is impossible to simulate all physics at all scales. For this reason, a wide ra
Externí odkaz:
http://arxiv.org/abs/2406.05901
Autor:
Racz, Istvan, Toth, Gabor Zsolt
Publikováno v:
Gen. Relativ. Gravit. 56 (2024) 131
The late-time behaviour of the solutions of the Fackerell-Ipser equation (which is a wave equation for the spin-zero component of the electromagnetic field strength tensor) on the closure of the domain of outer communication of sub-extremal Kerr spac
Externí odkaz:
http://arxiv.org/abs/2404.13447
Autor:
Chen, Yuxi, Toth, Gabor, Powell, Erick, Arshad, Talha, Bair, Ethan, Kornbleuth, Marc, Opher, Merav
The charge exchange between the interstellar medium (ISM) and the solar wind plasma is crucial for determining the structures of the heliosphere. Since both the neutral-ion and neutral-neutral collision mean free paths are either comparable to or lar
Externí odkaz:
http://arxiv.org/abs/2403.12395
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:
Huang, Zhenguang, Toth, Gabor, Huang, Jia, Sachdeva, Nishtha, van der Holst, Bart, Manchester, Ward B.
A potential field solution is widely used to extrapolate the coronal magnetic field above the Sun's surface to a certain height. This model applies the current-free approximation and assumes that the magnetic field is entirely radial beyond the sourc
Externí odkaz:
http://arxiv.org/abs/2403.01712
In a previous study, Huang et al. (2023) used the Alfven Wave Solar atmosphere Model (AWSoM), one of the widely used solar wind models in the community, driven by ADAPT-GONG magnetograms to simulate the solar wind in the last solar cycle and found th
Externí odkaz:
http://arxiv.org/abs/2403.01656
Gaussian Processes (GP) have become popular machine-learning methods for kernel-based learning on datasets with complicated covariance structures. In this paper, we present a novel extension to the GP framework using a contaminated normal likelihood
Externí odkaz:
http://arxiv.org/abs/2402.17570
Autor:
Shi, Chen, Velli, Marco, Toth, Gabor, Zhang, Kun, Tenerani, Anna, Huang, Zesen, Sioulas, Nikos, van der Holst, Bart
Publikováno v:
ApJL 964 L28 (2024)
Parker Solar Probe observations reveal that the near-Sun space is almost filled with magnetic switchbacks (``switchbacks'' hereinafter), which may be a major contributor to the heating and acceleration of solar wind. Here, for the first time, we deve
Externí odkaz:
http://arxiv.org/abs/2401.11334
Autor:
Zhao, Lulu, Sokolov, Igor, Gombosi, Tamas, Lario, David, Whitman, Kathryn, Huang, Zhenguang, Toth, Gabor, Manchester, Ward, van der Holst, Bart, Sachdeva, Nishtha
In this paper, we demonstrate the applicability of the data-driven and self-consistent solar energetic particle model, Solar-wind with FIeld-lines and Energetic-particles (SOFIE), to simulate acceleration and transport processes of solar energetic pa
Externí odkaz:
http://arxiv.org/abs/2309.16903