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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:scopusKinetic electrostatic waves and their association with current structures in the solar wind
ArticleAbstract: Context. A variety of kinetic electrostatic and electromagnetic waves develop in the solar wind andPalabras claves:solar wind, Turbulence, WavesAutores:Angelini V., Bale S.D., Chust T., Edberg N.J.T., Eriksson A.I., Evans V., Graham D.B., Horbury T.S., Johansson E.P.G., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Lorfèvre E., Luca Sorriso-Valvo, Maksimovic M., O'brien H., Píša D., Plettemeier D., Souček J., Steller M., Štverák , Trávníček P., Vaivads A., Vecchio A.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