10 citations · 10 across the 2 of their papers we have counts for
6 papers
In-situ Measurement of the Energy Fraction in Supra-thermal and Energetic Particles at ACE, Wind, and PSP Interplanetary Shocks
Liam David, Federico Fraschetti, Joe Giacalone +3
The acceleration of charged particles by interplanetary shocks (IPs) can drain a non-negligible fraction of the plasma pressure. In this study, we have selected 17 IPs observed in-…
Energy Balance at Interplanetary Shocks: In-situ Measurement of the Fraction in Supra-thermal and Energetic Particles with ACE and Wind
Liam David, Federico Fraschetti, Joe Giacalone +3
The acceleration of charged particles by interplanetary shocks can drain a non-negligible fraction of the upstream ram pressure. For a sample of shocks observed in-situ at 1 AU by…
Proton-proton collisional age to order solar wind types
Verena Heidrich-Meisner, Lars Berger, Robert F. Wimmer-Schweingruber
The properties of a solar wind stream are determined by its source region and by transport effects. Independently of the solar wind type, the solar wind measured in situ is always…
Disparity among low first ionization potential elements
Verena Heidrich-Meisner, Lars Berger, Robert F. Wimmer-Schweingruber
The elemental composition of the solar wind differs from the solar photospheric composition. Elements with low first ionization potential (FIP) appear enhanced compared to O in the…
Observations of high and low Fe charge states in individual solar wind streams with coronal-hole origin
Verena Heidrich-Meisner, Thies Peleikis, Martin Kruse +2
The solar wind originating from coronal holes is comparatively well-understood and is characterized by lower densities and average charge states compared to the so-called slow sola…
Evolution of an equatorial coronal hole structure and the released coronal hole wind stream: Carrington rotations 2039 to 2050
Verena Heidrich-Meisner, Thies Peleikis, Martin Kruse +2
The Sun is a highly dynamic environment that exhibits dynamic behavior on many different timescales. In particular, coronal holes exhibit temporal and spatial variability. Signatur…