Zobrazeno 1 - 10
of 112
pro vyhledávání: '"G. T. Taylor"'
Autor:
Arnaud Masson, C. Philippe Escoubet, Matthew G. G. T. Taylor, Detlef Sieg, Silvia Sanvido, Beatriz Abascal Palacios, Stijn Lemmens, Bruno Sousa
Publikováno v:
Earth, Planets and Space, Vol 76, Iss 1, Pp 1-20 (2024)
Abstract The Cluster mission will always be the first ever multi-spacecraft mission mapping the Earth magnetosphere in three dimensions. Launched in 2000 and originally planned to operate for two years, it has been orbiting Earth for more than two so
Externí odkaz:
https://doaj.org/article/97173ba0975c42478d562791125c44b8
Autor:
J. A. Carter, M. Dunlop, C. Forsyth, K. Oksavik, E. Donovon, A. Kavanagh, S. E. Milan, T. Sergienko, R. C. Fear, D. G. Sibeck, M. Connors, T. Yeoman, X. Tan, M. G. G. T. Taylor, K. McWilliams, J. Gjerloev, R. Barnes, D. D. Billet, G. Chisham, A. Dimmock, M. P. Freeman, D.-S. Han, M. D. Hartinger, S.-Y. W. Hsieh, Z.-J. Hu, M. K. James, L. Juusola, K. Kauristie, E. A. Kronberg, M. Lester, J. Manuel, J. Matzka, I. McCrea, Y. Miyoshi, J. Rae, L. Ren, F. Sigernes, E. Spanswick, K. Sterne, A. Steuwer, T. Sun, M.-T. Walach, B. Walsh, C. Wang, J. Weygand, J. Wild, J. Yan, J. Zhang, Q.-H. Zhang
Publikováno v:
Earth and Planetary Physics, Vol 8, Iss 1, Pp 275-298 (2024)
The joint European Space Agency and Chinese Academy of Sciences Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) mission will explore global dynamics of the magnetosphere under varying solar wind and interplanetary magnetic field conditions,
Externí odkaz:
https://doaj.org/article/29ec98756c3e4a33a1af2dd02c80e1c1
Autor:
Iannis Dandouras, Matt G. G. T. Taylor, Johan De Keyser, Yoshifumi Futaana, Ruth A. Bamford, Graziella Branduardi-Raymont, Jean-Yves Chaufray, Dragos Constantinescu, Elisabetta De Angelis, Pierre Devoto, Jonathan Eastwood, Marius Echim, Philippe Garnier, Benjamin Grison, David Hercik, Helmut Lammer, André Laurens, François Leblanc, Anna Milillo, Rumi Nakamura, Lubomír Přech, Elias Roussos, Štěpán Štverák, Julien Forest, Arnaud Trouche, Sébastien L. G. Hess, Jean-Charles Mateo-Vélez, James Carpenter, Josef Winter
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
The Lunar Orbital Platform - Gateway (LOP - Gateway, or simply Gateway) is a crewed platform that will be assembled and operated in the vicinity of the Moon by NASA and international partner organizations, including ESA, starting from the mid-2020s.
Externí odkaz:
https://doaj.org/article/36f7ce99177b45a286f1e08a4a2990e8
Autor:
C. Goetz, H. Gunell, F. Johansson, K. LLera, H. Nilsson, K.-H. Glassmeier, M. G. G. T. Taylor
Publikováno v:
Annales Geophysicae, Vol 39, Pp 379-396 (2021)
The plasma around comet 67P/Churyumov–Gerasimenko showed remarkable variability throughout the entire Rosetta mission. Plasma boundaries such as the diamagnetic cavity, solar wind ion cavity and infant bow shock separate regions with distinct plasm
Externí odkaz:
https://doaj.org/article/7f9fe8b18da04989bcb1803da9b3ac55
Autor:
T. Honig, O. G. Witasse, H. Evans, P. Nieminen, E. Kuulkers, M. G. G. T. Taylor, B. Heber, J. Guo, B. Sánchez-Cano
Publikováno v:
Annales Geophysicae, Vol 37, Pp 903-918 (2019)
The radiation data collected by the Standard Radiation Environment Monitor (SREM) aboard ESA missions INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory), Rosetta, Herschel, Planck and Proba-1, and by the high-energy neutron detector (HEND) in
Externí odkaz:
https://doaj.org/article/8db87c06690549a595ff7bec43394df4
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
Autor:
K. L. Heritier, K. Altwegg, J.-J. Berthelier, A. Beth, C. M. Carr, J. De Keyser, A. I. Eriksson, S. A. Fuselier, M. Galand, T. I. Gombosi, P. Henri, F. L. Johansson, H. Nilsson, M. Rubin, C. Simon Wedlund, M. G. G. T. Taylor, E Vigren
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-4 (2018)
Externí odkaz:
https://doaj.org/article/3ea8c28f054d432e80839324a31e74be
Publikováno v:
Geoscientific Instrumentation, Methods and Data Systems, Vol 5, Iss 2, Pp 289-304 (2016)
Astronauts on board the International Space Station (ISS) have taken thousands of high-resolution colour photographs of the aurora, which could be made useful for research if their pointing information could be reconstructed. We describe a method to
Externí odkaz:
https://doaj.org/article/8029956cb7a64508bee7d7eebc36753b
Autor:
Stephen E. Milan, Michaela K Mooney, Gemma E. Bower, Matthew G. G. T. Taylor, Larry J. Paxton, Iannis S Dandouras, Andrew Fazakerley, Christopher M. Carr, Brian J. Anderson, Sarah Kimberly Vines
We investigate a fifteen-day period in October 2011. Auroral observations by the SSUSI instrument onboard the DMSP F16, F17, and F18 spacecraft indicate that the polar regions were covered by weak cusp-aligned arc emissions whenever the IMF clock ang
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a46d86548776f7b59d503a0843ba9052
https://doi.org/10.22541/essoar.167690040.03060486/v1
https://doi.org/10.22541/essoar.167690040.03060486/v1
Autor:
Charlotte Goetz, Lucie Scharré, Cyril Simon Wedlund, Anja Moeslinger, Hans Nilsson, Elias Odelstad, Matthew G. G. T. Taylor, Martin Volwerk
The plasma environment at a comet can be divided into different regions with distinct plasma characteristics. Two such regions are the solar wind ion cavity, which refers to the part of the outer coma that does not contain any solar wind ions anymore
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79610a1a2cbb7defbafd0e9c05b3fd15
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-502681
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-502681