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Astronomy and Astrophysics(1)
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First Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source
ArticleAbstract: Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagatPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, Sun: general, TurbulenceAutores:André N., Angelini V., Bruno R., Coco I., De Marco R., D’Amicis R., Evans V., Fedorov A., Genot V., Horbury T.S., Jagarlamudi V.K., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Marcucci M.F., Matteini L., Müller D., O'brien H., Owen C.J., Panasenco O., Perrone D., Pezzi O., Rouillard A.P., Telloni D., Tenerani A., Velli M.C., Verscharen D., Woodham L.D., Zouganelis I.Fuentes:scopusDifferential kinetic dynamics and heating of ions in the turbulent solar wind
ArticleAbstract: The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solarPalabras claves:plasma heating, solar wind, space missions, TurbulenceAutores:Brienza D., Bruno R., Consolini G., de Keyser J., De Marco R., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Perrone D., Pezzi O., Retinò A., Salatti M., Servidio S., Stabile S., Vaivads A., Valentini F., Veltri P.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 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:scopus