Zobrazeno 1 - 10
of 554
pro vyhledávání: '"Lucek, E."'
The Interplanetary Magnetic Field shows complex spatial and temporal variations. Single spacecraft measurements reveal only a one dimensional section of this rich four dimensional phenomenon. Multi-point measurements of the four Cluster spacecraft pr
Externí odkaz:
http://arxiv.org/abs/1006.3239
Publikováno v:
Journal of Geophysical Research (Space Physics) 114, 11107, 2009
On 16 March 2005, the Cluster spacecraft crossed a shock almost at the transition between the quasi-perpendicular and quasi-parallel regimes ($\theta_{Bn}=46^{\circ}$) preceded by an upstream low-frequency ($\sim$ 0.02 Hz in the spacecraft frame) wav
Externí odkaz:
http://arxiv.org/abs/1001.5209
Autor:
Hietala, H., Laitinen, T. V., Andréeová, K., Vainio, R., Vaivads, A., Palmroth, M., Pulkkinen, T. I., Koskinen, H. E. J., Lucek, E. A., Rème, H.
The downstream region of a collisionless quasi-parallel shock is structured containing bulk flows with high kinetic energy density from a previously unidentified source. We present Cluster multi-spacecraft measurements of this type of supermagnetoson
Externí odkaz:
http://arxiv.org/abs/0911.1687
Autor:
Vörös, Z., Nakamura, R., Sergeev, V., Baumjohann, W., Runov, A., Zhang, T. L., Volwerk, M., Takada, T., Jankovičová, D., Lucek, E., Rème, H.
Publikováno v:
Journal of Geophysical Research, vol. 113, A07S29, 2008
The objective of the paper is to asses the specific spectral scaling properties of magnetic reconnection associated fluctuations/turbulence at the Earthward and tailward outflow regions observed simultaneously by the Cluster and Double Star (TC-2) sp
Externí odkaz:
http://arxiv.org/abs/0806.1829
Autor:
Xiao, C. J., Wang, X. G., Pu, Z. Y., Ma, Z. W., Zhao, H., Zhou, G. P., Wang, J. X., Kivelson, M. G., Fu, S. Y., Liu, Z. X., Zong, Q. G., Dunlop, M. W., Glassmeier, K-H., Lucek, E., Reme, H., Dandouras, I., Escoubet, C. P.
Publikováno v:
Nature Physics advance online publication, 24 June 2007
Detection of a separator line that connects magnetic nulls and the determination of the dynamics and plasma environment of such a structure can improve our understanding of the three-dimensional (3D) magnetic reconnection process. However, this type
Externí odkaz:
http://arxiv.org/abs/0705.1021
Autor:
Eastwood, J.1, Lucek, E.2, Mazelle, C.3, Meziane, K.4, Narita, Y.5, Pickett, J.6, Treumann, R.7
Publikováno v:
Space Science Reviews. May2005, Vol. 118 Issue 1-4, p41-94. 54p.
Autor:
Lucek, E.1, Constantinescu, D.2, Goldstein, M.3, Pickett, J.4, Pinçon, J.5, Sahraoui, F.6, Treumann, R.7, Walker, S.8
Publikováno v:
Space Science Reviews. May2005, Vol. 118 Issue 1-4, p95-152. 58p.
Autor:
Burgess, D.1, Lucek, E.2, Scholer, M.3, Bale, S.4, Balikhin, M.5, Balogh, A.2, Horbury, T.2, Krasnoselskikh, V.6, Kucharek, H.7, Lembège, B.8, Möbius, E., Schwartz, S., Thomsen, M.9, Walker, S.5
Publikováno v:
Space Science Reviews. May2005, Vol. 118 Issue 1-4, p205-222. 18p.
Publikováno v:
SCIENTIA SINICA Technologica. 40:757-764
Autor:
T.RUSSELL C., LUCEK E., FREY H., I.SAIFUDINOVA T., LARSON D., REME H., SIBECK D., ANGELOPOULOS V., MENDE S., A.SAPRONOVA L., MANN I., V.TOLOCHKO M., MCFADDEN J., MISHIN V., H.GLASSMEIER K.
Publikováno v:
SCIENTIA SINICA Technologica. 40:565-574