67 citations · 217 across the 7 of their papers we have counts for
7 papers
Helios 2 observations of solar wind turbulence decay in the inner heliosphere
Luca Sorriso-Valvo, Raffaele Marino, Foldes Raffaello +5
The linear scaling of the mixed third-order moment of the magnetohydrodynamic fluctuations is used to estimate the energy transfer rate of the turbulent cascade in the expanding so…
Modeling of Joint Parker Solar Probe - Metis/Solar Orbiter Observations
Laxman Adhikari, Gary P. Zank, Daniele Telloni +1
We present a first theoretical modeling of joint Parker Solar Probe (PSP) - Metis/Solar Orbiter (SolO) quadrature observations Telloni et al 2022c. The combined observations descri…
Turbulence/wave transmission at an ICME-driven shock observed by Solar Orbiter and Wind
L. L. Zhao, G. P. Zank, J. S. He +10
Solar Orbiter observed an interplanetary coronal mass ejection (ICME) event at 0.8 AU on 2020 April 19. The ICME was also observed by Wind at 1 AU on 2020 April 20. An interplaneta…
Linking Fluid and Kinetic Scales in Solar Wind Turbulence
D. Telloni, R. Bruno
We investigate possible links between the large-scale and small-scale features of solar wind fluctuations across the frequency break separating fluid and kinetic regimes. The aim i…
Spectral Features of Magnetic Fluctuations at Proton Scales from Fast to Slow Solar Wind
R. Bruno, D. Telloni
This Letter investigates the spectral characteristics of the interplanetary magnetic field fluctuations at proton scales during several time intervals chosen along the speed profil…
Detection of plasma fluctuations in white-light images of the outer solar corona: investigation of the spatial and temporal evolution
D. Telloni, R. Ventura, P. Romano +2
This work focus on the first results on the identification and characterization of periodic plasma density fluctuations in the outer corona, observed in STEREO-A COR1 white-light i…
Coronal Diagnostics from Narrowband Images around 30.4 nm
V. Andretta, D. Telloni, G. Del Zanna
Images taken in the band centered at 30.4 nm are routinely used to map the radiance of the He II Ly alpha line on the solar disk. That line is one of the strongest, if not the stro…