Extended magnetic reconnection at the Earth's magnetopause from detection of bi-directional jets

Magnetic reconnection is a process that converts magnetic energy into bi-directional plasma jets; it is believed to be the dominant process by which solar-wind energy enters the Earth's magnetosphere 1 , 2 . This energy is subsequently dissipated by magnetic storms and aurorae 3 , 4 . Previous...

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Veröffentlicht in:	Nature (London) 2000-04, Vol.404 (6780), p.848-850
Hauptverfasser:	Phan, T. D., Kistler, L. M., Klecker, B., Haerendel, G., Paschmann, G., Sonnerup, B. U. Ö., Baumjohann, W., Bavassano-Cattaneo, M. B., Carlson, C. W., DiLellis, A. M., Fornacon, K.-H., Frank, L. A., Fujimoto, M., Georgescu, E., Kokubun, S., Moebius, E., Mukai, T., Øieroset, M., Paterson, W. R., Reme, H.
Format:	Artikel
Sprache:	eng
Schlagworte:	Earth, ocean, space Exact sciences and technology External geophysics Humanities and Social Sciences Interaction between magnetosphere and interplanetary space Jets letter Magnetism multidisciplinary Physics of the magnetosphere Plasma Science Science (multidisciplinary) Solar energy Spacecraft Sun Wind power
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