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Turbulence 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:scopusScale-Dependent Kurtosis of Magnetic Field Fluctuations in the Solar Wind: A Multi-Scale Study With Cluster 2003–2015
ArticleAbstract: During the lifetime of the Cluster mission, the inter-spacecraft distances in the solar wind have chPalabras claves:Autores:Alexandrova O., Canu P., Escoubet C.P., Fischer D., Lion S., Luca Sorriso-Valvo, Nakamura R., Roberts O.W., Varsani A., Volwerk M., Vörös Z., Yearby K.Fuentes:scopus