activity
20162021
most citedHeliospheric Evolution of Magnetic Clouds

52 citations · 91 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202119 cited

Why are ELEvoHI CME arrival predictions different if based on STEREO-A or STEREO-B heliospheric imager observations?

Jürgen Hinterreiter, Tanja Amerstorfer, Martin A. Reiss +9

Accurate forecasting of the arrival time and arrival speed of coronal mass ejections (CMEs) is a unsolved problem in space weather research. In this study, a comparison of the pred…

physics.space-ph2020

Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations

Tanja Amerstorfer, Jürgen Hinterreiter, Martin A. Reiss +8

In this study, we evaluate a coronal mass ejection (CME) arrival prediction tool that utilizes the wide-angle observations made by STEREO's heliospheric imagers (HI). The unsurpass…

astro-ph.SR202019 cited

Prediction of Dst during solar minimum using in situ measurements at L5

R. L. Bailey, C. Möstl, M. A. Reiss +6

Geomagnetic storms resulting from high-speed streams can have significant negative impacts on modern infrastructure due to complex interactions between the solar wind and geomagnet…

physics.space-ph2020

Forecasting the Ambient Solar Wind with Numerical Models. II. An Adaptive Prediction System for Specifying Solar Wind Speed Near the Sun

Martin A. Reiss, Peter J. MacNeice, Karin Muglach +8

The ambient solar wind flows and fields influence the complex propagation dynamics of coronal mass ejections in the interplanetary medium and play an essential role in shaping Eart…

astro-ph.SR201952 cited

Heliospheric Evolution of Magnetic Clouds

Bojan Vršnak, Tanja Amerstorfer, Mateja Dumbović +7

Interplanetary evolution of eleven magnetic clouds (MCs) recorded by at least two radially aligned spacecraft is studied. The in situ magnetic field measurements are fitted to a cy…

astro-ph.SR20191 cited

EUV observations of cool dwarf stars

Allison Youngblood, Jeremy Drake, James Mason +15

The EUV (100-912 Å) is a spectral region notoriously difficult to observe due to attenuation by neutral hydrogen gas in the interstellar medium. Despite this, hundreds to thousands…