Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar
sidereal rotation period to proton and electron gyroperiods. Their amplitudes show …

Abstract Parker Solar Probe has been the first spacecraft to enter the deep corona below the
Alfvén critical point. Here we examine the higher-order statistical properties of magnetic-field …

At the end of 2020 September, the Parker Solar Probe (PSP) and BepiColombo were
radially aligned: PSP was orbiting near 0.17 au and BepiColombo near 0.6 au. This …

In this work, we investigate magnetic field fluctuations in three coronal mass ejection (CME)-
driven sheath regions at 1 AU, with their speeds ranging from slow to fast. The data set we …

Intermittency, an important property of astrophysical plasma turbulence, is studied
extensively during last decades from in-situ measurements of the solar wind plasma and …

Turbulent density fluctuations are investigated in the solar wind at sub-ion scales using
calibrated spacecraft potential. The measurement technique using the spacecraft potential …

Our previous studies have produced phenomenological models for turbulence in solar wind
plasmas on large-(inertial) magnetohydrodynamic scales, based on observations by the …

Combining the upstream solar wind observations measured by Mars Atmosphere and
Volatile Evolution (MAVEN), Advanced Composition Explorer (ACE) and Deep Space …

The solar wind is a highly turbulent medium, with a high level of field fluctuations throughout
a broad range of scales. These include an inertial range where a turbulent cascade is …

We present the multifractal study of the intermittency of the magnetic field turbulence in the
fast and slow solar wind beyond the ecliptic plane during two solar minima (1997–1998 …