Zobrazeno 1 - 10
of 94
pro vyhledávání: '"S. Toledo-Redondo"'
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 12, Pp n/a-n/a (2023)
Abstract Magnetic reconnection is a process that converts magnetic energy into kinetic energy, both bulk and thermal. We study the energy partition in magnetotail reconnection in the presence of cold ion populations of ionospheric origin using kineti
Externí odkaz:
https://doaj.org/article/b0887f9a240a4824afeb2b87dcb91d91
Autor:
A. Runov, M. Grandin, M. Palmroth, M. Battarbee, U. Ganse, H. Hietala, S. Hoilijoki, E. Kilpua, Y. Pfau-Kempf, S. Toledo-Redondo, L. Turc, D. Turner
Publikováno v:
Annales Geophysicae, Vol 39, Pp 599-612 (2021)
We present results of noon–midnight meridional plane global hybrid-Vlasov simulations of the magnetotail ion dynamics under a steady southward interplanetary magnetic field using the Vlasiator model. The simulation results show magnetotail reconnec
Externí odkaz:
https://doaj.org/article/3652868923354ed4b46191152677e3f8
Autor:
W. Y. Li, D. B. Graham, Yu. V. Khotyaintsev, A. Vaivads, M. André, K. Min, K. Liu, B. B. Tang, C. Wang, K. Fujimoto, C. Norgren, S. Toledo-Redondo, P.-A. Lindqvist, R. E. Ergun, R. B. Torbert, A. C. Rager, J. C. Dorelli, D. J. Gershman, B. L. Giles, B. Lavraud, F. Plaschke, W. Magnes, O. Le Contel, C. T. Russell, J. L. Burch
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-10 (2020)
Various types of plasma waves are generated around electron diffusion regions (EDRs). Here the authors show electron Bernstein waves (EBWs), at the electron-scale boundary of the Hall current reversal near EDR, are sufficiently strong to diffuse elec
Externí odkaz:
https://doaj.org/article/e3975f2c57c342b79a8fb72f9c6fd91f
Autor:
Z. Wang, X. Y. Liu, H. S. Fu, J. B. Cao, L. Dai, S. Toledo-Redondo, W. Z. Zhang, W. D. Fu, J. S. Zhao, Y. Yu, Z. Z. Guo
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 45 (2023)
Reconnection fronts, also known as dipolarization fronts (DFs), and kinetic Alfvén waves (KAWs) are two of the widely observed structures and waves in the terrestrial magnetotail, but their correlation remains elusive in previous spacecraft measurem
Externí odkaz:
https://doaj.org/article/8cb65183554642b4ab45b0cf65b3e1c5
Autor:
Yu-Xuan Li, Wen-Ya Li, Bin-Bin Tang, C. Norgren, Jian-Sen He, Chi Wang, Qiu-Gang Zong, S. Toledo-Redondo, M. André, C. Chappell, J. Dargent, S. A. Fuselier, A. Glocer, D. B. Graham, S. Haaland, L. Kistler, B. Lavraud, T. E. Moore, P. Tenfjord, S. K. Vines, J. Burch
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
Cold (few eV) ions of ionospheric origin are widely observed in the lobe region of Earth’s magnetotail and can enter the ion jet region after magnetic reconnection is triggered in the magnetotail. Here, we investigate a magnetotail crossing with co
Externí odkaz:
https://doaj.org/article/94c63b36483e4aa2a7a65c0c9dbc18d1
Autor:
Q. Lenouvel, V. Génot, P. Garnier, S. Toledo‐Redondo, B. Lavraud, N. Aunai, G. Nguyen, D. J. Gershman, R. E. Ergun, P.‐A. Lindqvist, B. Giles, J. L. Burch
Publikováno v:
Earth and Space Science, Vol 8, Iss 5, Pp n/a-n/a (2021)
Abstract This article presents 18 magnetic reconnection electron diffusion region (EDR) candidates found using a neural network algorithm with the Magnetospheric Multiscale Mission phase 1a data at the Earth's dayside magnetopause. These new candidat
Externí odkaz:
https://doaj.org/article/fa6a0894c3824c7f834248dfe4e93210
Publikováno v:
Geophysical Research Letters, Vol 47, Iss 4, Pp n/a-n/a (2020)
Abstract During periods of strong magnetic activity, cold dense plasma from the plasmasphere typically forms a plume extending toward the dayside magnetopause, eventually reaching it. In this work, we present a large‐scale two‐dimensional fully k
Externí odkaz:
https://doaj.org/article/0de2996b0aab433bbd02c1ec03f75688
Autor:
C. Philippe Escoubet, K.-J. Hwang, S. Toledo-Redondo, L. Turc, S. E. Haaland, N. Aunai, J. Dargent, Jonathan P. Eastwood, R. C. Fear, H. Fu, K. J. Genestreti, Daniel B. Graham, Yu V. Khotyaintsev, G. Lapenta, Benoit Lavraud, C. Norgren, D. G. Sibeck, A. Varsani, J. Berchem, A. P. Dimmock, G. Paschmann, M. Dunlop, Y. V. Bogdanova, Owen Roberts, H. Laakso, Arnaud Masson, M. G. G. T. Taylor, P. Kajdič, C. Carr, I. Dandouras, A. Fazakerley, R. Nakamura, Jim L. Burch, B. L. Giles, C. Pollock, C. T. Russell, R. B. Torbert
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 6 (2020)
When the supersonic solar wind encounters the Earth's magnetosphere a shock, called bow shock, is formed and the plasma is decelerated and thermalized in the magnetosheath downstream from the shock. Sometimes, however, due to discontinuities in the s
Externí odkaz:
https://doaj.org/article/b6152321939f425a81b2eb8cfee4636e
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Akademický článek
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