This paper focuses on the interactions between the fast solar wind from coronal holes and
the intervening slower solar wind, leading to the creation of stream interaction regions that …

The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

Aims. We study the evolution of stellar rotation and wind properties for low-mass main-
sequence stars. Our aim is to use rotational evolution models to constrain the mass loss …

In the past few years, several major space missions have been completed (eg, Deep Impact,
LCROSS, Chandrayaan-1, Stardust, Hayabusa), and a number of spacecraft are currently …

We analyze measured proton and electron temperatures in the high-speed solar wind in
order to calculate the separate rates of heat deposition for protons and electrons. When …

We measure the power and spectral index anisotropy of magnetic field fluctuations in fast
solar wind turbulence from scales larger than the outer scale down to the ion gyroscale, thus …

Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

Abstract As both Parker Solar Probe (PSP) and Solar Orbiter (SolO) reach heliocentric
distances closer to the Sun, they present an exciting opportunity to study the structure of …

The solar wind (SW) and the extreme ultraviolet (EUV) radiation modulate fluxes of
interstellar and heliospheric particles inside the heliosphere both in time and in space …

Magnetosheath jets are localized high‐dynamic pressure pulses originating at Earth's bow
shock and propagating earthward through the magnetosheath. Jets can influence …