The solar wind, a continuous flow of plasma from the sun, not only shapes the near Earth
space environment but also serves as a natural laboratory to study plasma turbulence in …

Interplanetary coronal mass ejections (ICMEs) have low proton beta across a broad range of
heliocentric distances and a magnetic flux rope structure at large scales, making them a …

The trace magnetic power spectrum in the solar wind is known to be characterized by a
double power law at scales much larger than the proton gyro-radius, with flatter spectral …

Using data from orbits 1− 11 of the Parker Solar Probe mission, the magnetic field spectral
index was measured across a range of heliocentric distances. The previously observed …

Context. The high Reynolds number solar wind flow provides a natural laboratory for the
study of turbulence in situ. Parker Solar Probe samples the solar wind between 0.17 AU and …

The nature of the Elsässer variable z− plays a significant role in the understanding of solar
wind turbulence. The radial spectral evolution of z− observed by the Helios spacecraft …

Magnetic fluctuations in the solar wind are often observed to maintain constant magnitude of
the magnetic field in a manner consistent with spherically polarized large-amplitude Alfvén …

Context. The nature and evolution of the solar wind magnetic field rotations is studied in data
from the Parker Solar Probe. Aims. We investigated the magnetic field deflections in the …

Alfvén waves, considered one of the primary candidates for heating and accelerating the fast
solar wind, are ubiquitous in spacecraft observations, yet their origin remains elusive. In this …

The highly Alfvénic fluctuations (AF) and magnetic-velocity alignment structures (MVAS) are
two distinguished components in the near-Sun slow solar wind observed by Parker Solar …