The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …

Turbulence in the solar wind can play essential roles in the heating of coronal and solar
wind plasma and the acceleration of the solar wind and energetic particles. Turbulence …

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 …

The scaling of the turbulent spectra provides a key measurement that allows us to
discriminate between different theoretical predictions of turbulence. In the solar wind, this …

The solar wind is a high Reynolds' number plasma flow of solar origin that permeates the
whole heliosphere. It is also the only accessible medium in which to study collisionless …

We employ a turbulence transport model to compute distributions of turbulence throughout
the heliosphere. The model determines the radial dependence of three (coupled) quantities …

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

The solar wind can be regarded as a turbulent magnetofluid, evolving in an expanding solar
wind and subject to turbulent driving by a variety of in situ sources. Furthermore, the solar …

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 Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
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