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The Fluid-like and Kinetic Behavior of Kinetic Alfvén Turbulence in Space Plasma
DOI: 10.3847/1538-4357/aaef77 Bibcode: 2019ApJ...870..106W

Verscharen, Daniel; Wicks, Robert T.; Chen, Christopher H. K. +3 more

Kinetic Alfvén waves (KAWs) are the short-wavelength extension of the magnetohydrodynamics Alfvén-wave branch in the case of highly oblique propagation with respect to the background magnetic field. Observations of space plasma show that small-scale turbulence is mainly KAW-like. We apply two theoretical approaches, a collisional two-fluid theory …

2019 The Astrophysical Journal
SolarOrbiter 21
The Impact of Turbulent Solar Wind Fluctuations on Solar Orbiter Plasma Proton Measurements
DOI: 10.3847/1538-4357/ab48e3 Bibcode: 2019ApJ...886..101N

Owen, C. J.; Nicolaou, G.; Verscharen, D. +1 more

Solar Orbiter will observe the Sun and the inner heliosphere to study the connections between solar activity, coronal structure, and the origin of the solar wind. The plasma instruments on board Solar Orbiter will determine the three-dimensional velocity distribution functions of the plasma ions and electrons with high time resolution. The analysi…

2019 The Astrophysical Journal
SolarOrbiter 19
Evolution of Coronal Mass Ejection Properties in the Inner Heliosphere: Prediction for the Solar Orbiter and Parker Solar Probe
DOI: 10.3847/1538-4357/ab4126 Bibcode: 2019ApJ...884..179A

Poedts, Stefaan; Lugaz, Noé; Al-Haddad, Nada +3 more

The evolution of the magnetic field and plasma quantities inside a coronal mass ejection (CME) with distance are known from statistical studies using data from 1 au monitors, planetary missions, Helios, and Ulysses. This does not cover the innermost heliosphere, below 0.29 au, where no data are yet publicly available. Here, we describe the evoluti…

2019 The Astrophysical Journal
SolarOrbiter 13