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The structure of magnetic turbulence in the heliosheath region observed by Voyager 2 at 106 AU
Conference ObjectAbstract: It is currently believed that the turbulent fluctuations pervade the outermost heliosphere. TurbulenPalabras claves:Autores:Federico Fraternale, Pogorelov N.V., Richagrdson J.D., Tordella D.Fuentes:scopusTransport of interstellar neutral helium throughout the heliosphere
ArticleAbstract: A number of physical processes accompanying the solar wind interaction with the local interstellar mPalabras claves:Astrosphere interstellar medium interactions (106), Charge exchange ionization (2056), Heliopause (707), Heliosphere (711), Interstellar atomic gas (833), Interstellar medium (847), Interstellar plasma (851)Autores:Federico Fraternale, Heerikhuisen J., Pogorelov N.V.Fuentes:scopusTurbulence in the Outer Heliosphere
ReviewAbstract: The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is gPalabras claves:Heliosphere, Interstellar medium, solar wind, TurbulenceAutores:Adhikari L., Charles W. Smith, Federico Fraternale, Fichtner H., Kim T.K., Kleimann J., Oughton S., Pogorelov N.V., Roytershteyn V., Smith C.W., Tae K. Kim, Usmanov A.V., Zank G.P., Zhao L.L.Fuentes:scopusTurbulence in the solar wind: Spectra from Voyager 2 data at 5 AU
OtherAbstract: Fluctuations in the flow velocity and magnetic fields are ubiquitous in the Solar System. These flucPalabras claves:data gap, data recovery, solar wind turbulence, Spectral Analysis, Voyager 2Autores:Federico Fraternale, Gallana L., Iovieno M., Opher M., Richardson J.D., Tordella D.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:scopusSolar wind spectral analysis in heliosheath from Voyager 2 data
Conference ObjectAbstract: The solar wind is a supersonic flow of magnetized plasma. It is time-dependent on all scales and expPalabras claves:Autores:Federico Fraternale, Fosson S.M., Gallana L., Iovieno M., Magli E., Opher M., Richardson J.D., Tordella D.Fuentes:scopusThe Global Structure of the Heliosphere
ArticleAbstract: As the Sun moves through the local interstellar medium (LISM), it emits charged particles, creatingPalabras claves:Autores:Federico Fraternale, Pogorelov N.V., Zank G.P., Zhang M.Fuentes:scopusThe Role of Pickup Ions in the Interaction of the Solar Wind with the Local Interstellar Medium. II. Effects of Solar Cycle
ArticleAbstract: We investigate the role of pickup ions (PUIs) in the interaction of a periodically varying solar winPalabras claves:Autores:Federico Fraternale, M. Gedalin, Pogorelov N.V., R. K. Bera, Roytershteyn V., Zank G.P.Fuentes:scopusFluctuations Driven by Multicomponent Pickup Ion Distributions in the Outer Heliosheath
ArticleAbstract: The stability of a realistic multicomponent pickup ion (PUI) velocity distribution derived from a glPalabras claves:Autores:Ameneh Mousavi, Federico Fraternale, Pogorelov N.V., Roytershteyn V.Fuentes:scopusMagnetohydrodynamic/Kinetic Modeling of the Interaction between the Solar Wind and the Local Interstellar Medium with He+, He2+, and Pickup H+ ions and H, He Atoms
OtherAbstract: The interaction of the solar wind with the local interstellar medium (LISM) spans a wide range of inPalabras claves:Autores:Federico Fraternale, Pogorelov N.V., R. K. BeraFuentes:scopus