Zobrazeno 1 - 10
of 5 290
pro vyhledávání: '"TÓTH, G."'
Autor:
Kornbleuth, M., Opher, M., Baliukin, I., Gkioulidou, M., Richardson, J. D., Zank, G. P., Michael, A. T., Toth, G., Tenishev, V., Izmodenov, V., Alexashov, D., Fuselier, S., Drake, J. F., Dialynas, K.
Global models of the heliosphere are critical tools used in the interpretation of heliospheric observations. There are several three-dimensional magnetohydrodynamic (MHD) heliospheric models that rely on different strategies and assumptions. Until no
Externí odkaz:
http://arxiv.org/abs/2110.13962
Autor:
Kornbleuth, M., Opher, M., Michael, A. T., Sokol, J. M., Toth, G., Tenishev, V., Drake, J. F.
Traditionally, the solar magnetic field has been considered to have a negligible effect in the outer regions of the heliosphere. Recent works have shown that the solar magnetic field may play a crucial role in collimating the plasma in the heliosheat
Externí odkaz:
http://arxiv.org/abs/2005.06643
We present a novel algorithm that predicts the probability that the time derivative of the horizontal component of the ground magnetic field $dB/dt$ exceeds a specified threshold at a given location. This quantity provides important information that
Externí odkaz:
http://arxiv.org/abs/1912.01038
Autor:
Moschou, S. P., Sokolov, I. V., Cohen, O., Toth, G., Drake, J. J., Huang, Z., Garraffo, C., Alvarado-Gómez, J. D., Gombosi, T.
Heliospheric plasmas require multi-scale and multi-physics considerations. On one hand, MHD codes are widely used for global simulations of the solar-terrestrial environments, but do not provide the most elaborate physical description of space plasma
Externí odkaz:
http://arxiv.org/abs/1911.08660
Autor:
Sachdeva, N., van der Holst, B., Manchester, W. B., Tóth, G., Chen, Y., Lloveras, D. G., Vásquez, A. M., Lamy, Philippe, Wojak, Julien, Jackson, B. V., Yu, H. -S., Henney, C. J.
We perform a validation study of the latest version of the Alfv\'{e}n Wave Solar atmosphere Model (AWSoM) within the Space Weather Modeling Framework (SWMF). To do so, we compare the simulation results of the model with a comprehensive suite of obser
Externí odkaz:
http://arxiv.org/abs/1910.08110
Akademický článek
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Autor:
Huang, Z., Toth, G., Gombosi, T. I., Jia, X., Combi, M. R., Hansen, K. C., Fougere, N., Shou, Y., Tenishev, V., Altwegg, K., Rubin, M.
Publikováno v:
Published in MNRAS in 2018
Magnetohydrodynamics simulations have been carried out in studying the solar wind and cometary plasma interactions for decades. Various plasma boundaries have been simulated and compared well with observations for comet 1P/Halley. The Rosetta mission
Externí odkaz:
http://arxiv.org/abs/1801.03991
Autor:
Csilla, Obádovics1 obadovics.csilla@uni-sopron.hu, Csaba, Tóth. G.2 toth.gcsaba@krtk.hu
Publikováno v:
Hungarian Statistical Review / Statisztikai Szemle. sze2023, Vol. 101 Issue 9, p763-792. 30p.
Autor:
Tóth, G. Csaba
Publikováno v:
Corvinus Journal of Sociology and Social Policy. 13(1):161-166
Externí odkaz:
https://www.ceeol.com/search/article-detail?id=1067206
Given a sequence $S=(s_1,\dots,s_m) \in [0, 1]^m$, a block $B$ of $S$ is a subsequence $B=(s_i,s_{i+1},\dots,s_j)$. The size $b$ of a block $B$ is the sum of its elements. It is proved in [1] that for each positive integer $n$, there is a partition o
Externí odkaz:
http://arxiv.org/abs/1706.06095