The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
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This statistical analysis of power spectra of the fluctuating Elsässer variables, δZ±= δV±δVA,
covers 3408 hours of interplanetary magnetic field and plasma observations made by …

We examine the radial evolution of correlation lengths perpendicular (${\lambda} _
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …

Physics of the Inner Heliosphere gives for the first time a comprehensive and complete
summary of our knowledge of the inner solar system. Using data collected over more than …

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 …

At the end of 1992, the Pioneer 10, Pioneer 11, and Voyager 2 spacecraft were at
heliocentric distances of 56.0, 37.3, and 39.0 AU and heliographic latitudes of 3.3° N, 17.4° …

Using hour‐averaged data from the Helios and Voyager spacecraft, we have investigated
the origin and evolution of low‐frequency interplanetary fluctuations from 0.3 to 20 AU …

We have developed an axisymmetric steady-state solar wind model that describes
properties of the large-scale solar wind, interplanetary magnetic field, and turbulence …

We present a study of the variation of the relative abundance of helium to hydrogen in the
solar wind as a function of solar wind speed and heliographic latitude over the previous …

The fourth orbit of Parker Solar Probe (PSP) reached heliocentric distances down to 27.9
R⊙, allowing solar wind turbulence and acceleration mechanisms to be studied in situ …