Zobrazeno 1 - 10
of 4 965
pro vyhledávání: '"Toth, G"'
Autor:
Fougere, Nicolas, Altwegg, K., Berthelier, J.-J., Bieler, A., Bockelée-Morvan, D., Calmonte, U., Capaccioni, F., Combi, M. R., De Keyser, J., Debout, V., Erard, S., Fiethe, B., Filacchione, G., Fink, U., Fuselier, S. A., Gombosi, T. I., Hansen, K. C., Hässig, M., Huang, Z., Le Roy, L., Leyrat, C., Migliorini, A., Piccioni, G., Rinaldi, G., Rubin, M., Shou, Y., Tenishev, V., Toth, G., Tzou, C.-Y.
We analyse the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) - the Double Focusing Mass Spectrometer data between 2014 August and 2016 February to examine the effect of seasonal variations on the four major species within the com
Externí odkaz:
http://hdl.handle.net/10150/624746
http://arizona.openrepository.com/arizona/handle/10150/624746
http://arizona.openrepository.com/arizona/handle/10150/624746
Autor:
Fougere, N., Altwegg, K., Berthelier, J.-J., Bieler, A., Bockelée-Morvan, D., Calmonte, U., Capaccioni, F., Combi, M. R., De Keyser, J., Debout, V., Erard, S., Fiethe, B., Filacchione, G., Fink, U., Fuselier, S. A., Gombosi, T. I., Hansen, K. C., Hässig, M., Huang, Z., Le Roy, L., Leyrat, C., Migliorini, A., Piccioni, G., Rinaldi, G., Rubin, M., Shou, Y., Tenishev, V., Toth, G., Tzou, C.-Y.
Context. Since its rendezvous with comet 67P/Churyumov-Gerasimenko (67P), the Rosetta spacecraft has provided invaluable information contributing to our understanding of the cometary environment. On board, the VIRTIS and ROSINA instruments can both m
Externí odkaz:
http://hdl.handle.net/10150/614711
http://arizona.openrepository.com/arizona/handle/10150/614711
http://arizona.openrepository.com/arizona/handle/10150/614711
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
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