The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

While it is certain that the fast solar wind originates from coronal holes, where and how the
slow solar wind (SSW) is formed remains an outstanding question in solar physics even in …

A major challenge for gravitational-wave (GW) detection in the μ Hz band is engineering a
test mass (TM) with sufficiently low acceleration noise. We propose a GW detection concept …

The long-anticipated encounter by Voyager 2 (V2) of the region between the heliosphere
and the very local interstellar medium (VLISM) occurred toward the end of 2018. Here, we …

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 …

Abstract NASA's Interstellar Boundary Explorer (IBEX) mission has operated in space for a
full solar activity cycle (Solar Cycle 24), and IBEX observations have exposed the global …

Abstract The Interstellar Boundary Explorer (IBEX) has now operated in space for 7 years
and returned nearly continuous observations that have led to scientific discoveries and …

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 …

The solar wind (SW) is an outflow of the solar coronal plasma, which expands
supersonically throughout the heliosphere. SW particles interact by charge exchange with …

Computer-assisted tomography (CAT) for interplanetary scintillation (IPS) observations
enables the determination of the global distribution of solar wind speed. We compared solar …