Evolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe–Solar Orbiter Radial Alignment
The first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used
to investigate the evolution of solar wind turbulence in the inner heliosphere. Assuming …
to investigate the evolution of solar wind turbulence in the inner heliosphere. Assuming …
Impact of switchbacks on turbulent cascade and energy transfer rate in the inner heliosphere
CS Hernández, L Sorriso-Valvo… - The Astrophysical …, 2021 - iopscience.iop.org
Abstract Recent Parker Solar Probe (PSP) observations of inner heliospheric plasma have
shown an abundant presence of Alfvénic polarity reversal of the magnetic field, known as" …
shown an abundant presence of Alfvénic polarity reversal of the magnetic field, known as" …
Turbulent cascade and energy transfer rate in a solar coronal mass ejection
L Sorriso-Valvo, E Yordanova… - The Astrophysical …, 2021 - iopscience.iop.org
Turbulence properties are examined before, during, and after a coronal mass ejection
(CME) detected by the Wind spacecraft in 2012 July. The power-law scaling of the structure …
(CME) detected by the Wind spacecraft in 2012 July. The power-law scaling of the structure …
Helios 2 observations of solar wind turbulence decay in the inner heliosphere
Aims. A linear scaling of the mixed third-order moment of the magnetohydrodynamic (MHD)
fluctuations is used to estimate the energy transfer rate of the turbulent cascade in the …
fluctuations is used to estimate the energy transfer rate of the turbulent cascade in the …
Comparing turbulence in a Kelvin–Helmholtz instability region across the terrestrial magnetopause
P Quijia, F Fraternale, JE Stawarz… - Monthly Notices of …, 2021 - academic.oup.com
The properties of turbulence observed within the plasma originating from the
magnetosheath and the magnetospheric boundary layer, which have been entrained within …
magnetosheath and the magnetospheric boundary layer, which have been entrained within …
Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations
Context. The recently released spacecraft potential measured by the RPW instrument on
board Solar Orbiter has been used to estimate the solar wind electron density in the inner …
board Solar Orbiter has been used to estimate the solar wind electron density in the inner …
Turbulence and particle energization in twisted flux ropes under solar-wind conditions
Context. The mechanisms regulating the transport and energization of charged particles in
space and astrophysical plasmas are still debated. Plasma turbulence is known to be a …
space and astrophysical plasmas are still debated. Plasma turbulence is known to be a …
Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data
An MHD shell model is used to describe the dissipative events that take place in magnetized
plasmas. We analyze the activity of the time series of the magnetic energy dissipation rate …
plasmas. We analyze the activity of the time series of the magnetic energy dissipation rate …
Sign singularity of the local energy transfer in space plasma turbulence
L Sorriso-Valvo, G De Vita, F Fraternale… - Frontiers in …, 2019 - frontiersin.org
In weakly collisional space plasmas, the turbulent cascade provides most of the energy that
is dissipated at small scales by various kinetic processes. Understanding the characteristics …
is dissipated at small scales by various kinetic processes. Understanding the characteristics …
Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection
R Márquez Rodríguez, L Sorriso-Valvo, E Yordanova - Solar Physics, 2023 - Springer
Solar wind measurements carried out by NASA's Wind spacecraft before, during, and after
the passing of an interplanetary coronal mass ejection (ICME), detected on 12–14 …
the passing of an interplanetary coronal mass ejection (ICME), detected on 12–14 …