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EIDOSCOPE: Particle acceleration at plasma boundaries
ArticleAbstract: We describe the mission concept of how ESA can make a major contribution to the Japanese Canadian muPalabras claves:Cosmic vision, Multi-scale coupling in plasmas, Particle acceleration, Space plasmasAutores:Andersson G., Bale S.D., Cully C.M., de Keyser J., Fujimoto M., Grahn S., Haaland S., Ji H., Khotyaintsev Y.V., Lavraud B., Lazarian A., Luca Sorriso-Valvo, Mann I.R., Nakamura R., Nakamura T.K.M., Narita Y., Retinò A., Sahraoui F., Schekochihin A., Schwartz S.J., Shinohara I., Vaivads A.Fuentes:scopusParticle energization in space plasmas: towards a multi-point, multi-scale plasma observatory
ArticleAbstract: This White Paper outlines the importance of addressing the fundamental science theme “How are chargePalabras claves:Astrophysical Plasmas, Heliosphere, Particle energization, Scale coupling, Space plasmas, Spacecraft constellationsAutores:Angelopoulos V., Blasi P., Burch J.L., Dai L., de Keyser J., Dunlop M., Eastwood J.P., Fu H., Haaland S., Hoshino M., Johlander A., Kepko L., Khotyaintsev Y.V., Kucharek H., Lapenta G., Lavraud B., Le Contel O., Luca Sorriso-Valvo, Malandraki O.E., Marcucci M.F., Matthaeus W.H., McWilliams K., Petrukovich A., Pinçon J.L., Plaschke F., Retinò A., Saito Y., Vainio R., Vaivads A., Wimmer-Schweingruber R.F.Fuentes:scopusTurbulence-Driven Ion Beams in the Magnetospheric Kelvin-Helmholtz Instability
ArticleAbstract: The description of the local turbulent energy transfer and the high-resolution ion distributions meaPalabras claves:Autores:Burch J.L., Carbone V., Catapano F., Coburn J.T., Di Mare F., Federico Fraternale, Giles B.L., Greco A., Khotyaintsev Y.V., Le Contel O., Luca Sorriso-Valvo, Malara F., Moore T.E., Panebianco V., Perri S., Perrone D., Pezzi O., Raffaele Marino, Retinò A., Roberts O.W., Russell C.T., Torbert R.B., Valentini F., Veltri P.Fuentes:scopusTHIN CURRENT SHEETS AND ASSOCIATED ELECTRON HEATING IN TURBULENT SPACE PLASMA
ArticleAbstract: Intermittent structures, such as thin current sheets, are abundant in turbulent plasmas. Numerical sPalabras claves:acceleration of particles, Magnetic fields, magnetic reconnection, plasmas, TurbulenceAutores:Canu P., Chasapis A., Greco A., Khotyaintsev Y.V., Luca Sorriso-Valvo, Retinò A., Sahraoui F., Sundkvist D., Vaivads A.Fuentes:scopus