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scopus(3)
Cancellation analysis of current density in solar active region NOAA10019
ArticleAbstract: Solar flares are often associated with changes in the fine magnetic structure of the emitting activePalabras claves:Active regions, Photosphere, Solar flaresAutores:Briand C., Carbone V., De Vita G., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A.Fuentes:scopusTurbulence Heating ObserveR - Satellite mission proposal
ArticleAbstract: The Universe is permeated by hot, turbulent, magnetized plasmas. Turbulent plasma is a major constitPalabras claves:plasma heating, plasma properties, Space plasma physicsAutores:Alexandrova O., André M., Bale S.D., Balikhin M., Burgess D., Camporeale E., Caprioli D., Chen C.H.K., Clacey E., Cully C.M., de Keyser J., Eastwood J.P., Eriksson S., Escoubet C.P., Fazakerley A.N., Goldstein M.L., Graham D.B., Haaland S., Hoshino M., Ji H., Karimabadi H., Khotyaintsev Y.V., Kucharek H., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Matthaeus W.H., Moore T.E., Nakamura R., Narita Y., Nemecek Z., Norgren C., Opgenoorth H., Palmroth M., Perrone D., Pinçon J.L., Rathsman P., Retinò A., Rothkaehl H., Sahraoui F., Servidio S., Souček J., Vainio R., Vaivads A., Valentini F., Vörös Z., Wimmer-Schweingruber R.F.Fuentes:scopusProperties of Turbulence in the Reconnection Exhaust: Numerical Simulations Compared with Observations
ArticleAbstract: The properties of the turbulence that develops in the outflows of magnetic reconnection have been inPalabras claves:magnetic reconnection, methods: numerical, TurbulenceAutores:Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Malara F., Matthaeus W.H., Newman D.L., Olshevsky V., Pucci F., Servidio S.Fuentes:scopus