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 …
Spectral features in field-aligned solar wind turbulence from Parker Solar Probe observations
LL Zhao, GP Zank, L Adhikari… - The Astrophysical …, 2020 - iopscience.iop.org
Abstract Parker Solar Probe (PSP) observed a large variety of Alfvénic fluctuations in the fast
and slow solar wind flow during its two perihelia. The properties of Alfvénic solar wind …
and slow solar wind flow during its two perihelia. The properties of Alfvénic solar wind …
Magnetic field intermittency in the solar wind: Parker solar probe and SolO observations ranging from the alfvén region up to 1 AU
Abstract Parker Solar Probe (PSP) and SolO data are utilized to investigate magnetic field
intermittency in the solar wind (SW). Small-scale intermittency (20− 100 di) is observed to …
intermittency in the solar wind (SW). Small-scale intermittency (20− 100 di) is observed to …
Density fluctuations associated with turbulence and waves-First observations by Solar Orbiter
Aims. The aim of this work is to demonstrate that the probe-to-spacecraft potential measured
by RPW on Solar Orbiter can be used to derive the plasma (electron) density measurement …
by RPW on Solar Orbiter can be used to derive the plasma (electron) density measurement …
No evidence for critical balance in field-aligned Alfvénic solar wind turbulence
The properties of Alfvénic solar wind turbulence have been studied for decades using
spacecraft measurements. In particular, the observation of spectral anisotropy of magnetic …
spacecraft measurements. In particular, the observation of spectral anisotropy of magnetic …
A comprehensive power spectral density analysis of astronomical time series. I. The Fermi-LAT gamma-ray light curves of selected blazars
M Tarnopolski, N Żywucka, V Marchenko… - The Astrophysical …, 2020 - iopscience.iop.org
We present the results of the Fermi-Large Area Telescope 10 yr long light curve (LC)
modeling of selected blazars: six flat-spectrum radio quasars (FSRQs) and five BL Lacertae …
modeling of selected blazars: six flat-spectrum radio quasars (FSRQs) and five BL Lacertae …
High-frequency magnetic fluctuations in space plasmas and the role of electron Landau damping
While low-frequency plasma fluctuations in the interplanetary space have been successfully
described in the framework of classical turbulence, high-frequency fluctuations still represent …
described in the framework of classical turbulence, high-frequency fluctuations still represent …
Multifractal and chaotic properties of solar wind at MHD and kinetic domains: An empirical mode decomposition approach
Turbulence, intermittency, and self-organized structures in space plasmas can be
investigated by using a multifractal formalism mostly based on the canonical structure …
investigated by using a multifractal formalism mostly based on the canonical structure …
Coherent events at ion scales in the inner heliosphere: Parker solar probe observations during the first encounter
Abstract The Parker Solar Probe mission has shown the ubiquitous presence of strong
magnetic field deflections, namely switchbacks, during its first perihelion where it was …
magnetic field deflections, namely switchbacks, during its first perihelion where it was …
On the scaling properties of magnetic-field fluctuations through the inner heliosphere
Although the interplanetary magnetic-field variability has been extensively investigated in
situ using data from several space missions, newly launched missions providing high …
situ using data from several space missions, newly launched missions providing high …