activity
20182022
most citedHow the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth -- An analytical model

24 citations · 37 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202224 cited

How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth -- An analytical model

Stefan Johann Hofmeister, Eleanna Asvestari, Jingnan Guo +10

We derive a simple analytical model for the propagation of HSSs from the Sun to Earth and thereby show how the area of coronal holes and the size of their boundary regions affect t…

astro-ph.SR202013 cited

An elliptic expansion of the potential field source surface model

Martin Kruse, Verena Heidrich-Meisner, R. F. Wimmer-Schweingruber +1

Context. The potential field source surface model is frequently used as a basis for further scientific investigations where a comprehensive coronal magnetic field is of importance.…

astro-ph.SR2020

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…

astro-ph.SR2018

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…

physics.space-ph2018

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…

physics.space-ph2018

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…