Mostrando 10 resultados de: 13
Filtros aplicados
Publisher
Astronomy and Astrophysics(4)
Astrophysical Journal(2)
Astrophysical Journal Letters(2)
Physical Review Letters(2)
Earth, Planets and Space(1)
Área temáticas
Cuerpos y fenómenos celestes específicos(7)
Mecánica de fluidos(3)
Geología, hidrología, meteorología(2)
Astronomía y ciencias afines(1)
Ciencias de la tierra(1)
Área de conocimiento
Viento solar(5)
Energía solar(3)
Magnetohidrodinámica(2)
Ciencia atmosférica(1)
Fenómenos de transporte(1)
Origen
scopus(13)
Frequency spectra of horizontal winds in the mesosphere and lower thermosphere region from multistatic specular meteor radar observations during the SIMONe 2018 campaign
ArticleAbstract: In recent years, multistatic specular meteor radars (SMRs) have been introduced to study the MesosphPalabras claves:Frequency spectra, Horizontal winds, mesosphere and lower thermosphere, SIMONe 2018, specular meteor radar, Wind field Correlation Function InversionAutores:Charuvil Asokan H., Chau J.L., Clahsen M., Jacobi C., Raffaele Marino, Urco J.M., Vargas F., Vierinen J.Fuentes:scopusFirst polar observations of the fast solar wind with the Metis Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration
ArticleAbstract: Context. The fast solar wind is known to emanate from polar coronal holes. Aims. This Letter reportsPalabras claves:magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: UV radiationAutores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Capuano G.E., De Leo Y., Deppo V.D., D’Amicis R., Fineschi S., Giordano S., Grimani C., Heinzel P., Jerse G., Landini F., Liberatore A., Luca Sorriso-Valvo, Moses J.D., Naletto G., Nicolini G., Pancrazzi M., Perrone D., Raffaele Marino, Romoli M., Russano G., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Uslenghi M., Vai M., Zank G.P., Zhao L.L.Fuentes:scopusErratum: Comparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stab319)
OtherAbstract: The original version of this manuscript included some portions of text from the first submitted versPalabras claves:Autores:Christian L. Vásconez, Federico Fraternale, Luca Sorriso-Valvo, Paulina Quijia, Perri S., Raffaele Marino, Stawarz J.E., Yordanova E.Fuentes:scopusEvolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe-Solar Orbiter Radial Alignment
ArticleAbstract: The first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used to investPalabras claves:Autores:Adhikari L., Angelini V., Antonucci E., Bale S.D., Bruno R., Carbone F., Case A.W., De Marco R., Dudok De Wit T., D’Amicis R., Evans V., Goetz K., Harvey P.R., Horbury T.S., Jagarlamudi V.K., Kasper J.C., Korreck K.E., Laker R., Larson D., Liang H., Livi R., Livi S., Louarn P., Luca Sorriso-Valvo, Macdowall R.J., Malaspina D.M., Nakanotani M., O'brien H., Owen C.J., Panasenco O., Perrone D., Pulupa M., Raffaele Marino, Romoli M., Shi C., Steinvall K., Stevens M.L., Telloni D., Tenerani A., Velli M.C., Whittlesey P., Woodham L.D., Zank G.P., Zhao L.L.Fuentes:scopusHeating the solar wind by a magnetohydrodynamic turbulent energy cascade
ArticleAbstract: Solar wind plasma is known to cool down more slowly while it is blown away from the Sun than expectePalabras claves:MHD, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusHelios 2 observations of solar wind turbulence decay in the inner heliosphere
ArticleAbstract: Aims. A linear scaling of the mixed third-order moment of the magnetohydrodynamic (MHD) fluctuationsPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Bruno R., D,Aamicis R., Foldes R., Lévêque E., Luca Sorriso-Valvo, Raffaele Marino, Telloni D., Yordanova E.Fuentes:scopusObservation and Modeling of the Solar Wind Turbulence Evolution in the Sub-Mercury Inner Heliosphere
ArticleAbstract: This letter exploits the radial alignment between the Parker Solar Probe and BepiColombo in late 202Palabras claves:Autores:Adhikari L., Alberti T., Auster H.U., Bale S.D., Bruno R., Califano F., Carbone F., Case A.W., Dudok De Wit T., D’Amicis R., Goetz K., Grimani C., Hadid L.Z., Harvey P.R., Heyner D., Kasper J.C., Korreck K.E., Laker R., Larson D., Liberatore A., Livi R., Luca Sorriso-Valvo, Macdowall R.J., Malara F., Malaspina D.M., Milillo A., Narita Y., Panasenco O., Perrone D., Pulupa M., Raffaele Marino, Richter I., Sánchez-Cano B., Shi C., Stawarz J.E., Stevens M.L., Susino R., Telloni D., Velli M.C., Verdini A., Verscharen D., Whittlesey P., Zank G.P., Zhao L.L.Fuentes:scopusObservation of inertial energy cascade in interplanetary space plasma
ArticleAbstract: Direct evidence for the presence of an inertial energy cascade, the most characteristic signature ofPalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Lepreti F., Luca Sorriso-Valvo, Noullez A., Pietropaolo E., Raffaele Marino, Veltri P.Fuentes:scopusLinking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations
ArticleAbstract: The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in coPalabras claves:Autores:Abbo L., Adhikari L., Andretta V., Auchère F., Bale S.D., Berlicki A., Biondo R., Bruno R., Capobianco G., Capuano G.E., Carbone F., Case A.W., Casini C., Casti M., Chioetto P., Ciaravella A., Corso A.J., Cuadrado R.A., Deppo V.D., Dudok De Wit T., D’Amicis R., Fabi M., Fineschi S., Frassati F., Frassetto F., Giordano S., Goetz K., Grimani C., Guglielmino S.L., Hadid L.Z., Harvey P.R., Heinzel P., Jerse G., Kasper J.C., Korreck K.E., Lamy P., Landini F., Lanzafame A., Larson D., Leo Y.D., Liang H., Liberatore A., Livi R., Luca Sorriso-Valvo, Macdowall R.J., Magli E., Malaspina D.M., Malvezzi M., Mancuso S., Massone G., Messerotti M., Moses J.D., Nakanotani M., Naletto G., Nicolini G., Nicolosi P., Nisticò G., Pagano P., Panasenco O., Pancrazzi M., Pelizzo M.G., Perrone D., Peter H., Pulupa M., Raffaele Marino, Reale F., Romano P., Romoli M., Sánchez-Cano B., Sasso C., Schühle U., Slemer A., Solanki S.K., Spadaro D., Stangalini M., Stevens M.L., Strachan L., Straus T., Susino R., Telloni D., Teriaca L., Tsinganos K., Uslenghi M., Velli M.C., Ventura R., Verscharen D., Vial J.C., Volpicelli C.A., Whittlesey P., Woch J., Zangrilli L., Zank G.P., Zhao L.L., Zimbardo G., Zuppella P.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:scopus