105 citations
- Austrian Academy of SciencesAT2 papers
- Goddard Space Flight CenterUS2 papers
- Space Research InstituteRU2 papers
- University of GrazAT2 papers
- Community Coordinated Modeling Center1 paper
- Graz University of TechnologyAT1 paper
- HeliophysicsUS1 paper
- Helmholtz Institute Freiberg for Resource TechnologyDE1 paper
- Helmholtz-Zentrum Dresden-RossendorfDE1 paper
- Predictive Science (United States)US1 paper
- Rutherford Appleton LaboratoryGB1 paper
- Technical University of MunichDE1 paper
5 papers
Which Upstream Solar Wind Conditions Matter Most in Predicting Bz within Coronal Mass Ejections
Pete Riley, M. A. Reiss, C. Mostl
Accurately predicting the z-component of the interplanetary magnetic field, particularly during the passage of an interplanetary coronal mass ejection (ICME), is a crucial objectiv…
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…
Assimilation of the SCATSAR-SWI with SURFEX: Impact of local observation errors in Austria
J. Vural, S. Schneider, B. Bauer-Marschallinger +1
The proper determination of soil moisture on different scales is important for applications in a variety of fields. We aim to develop a high-level soil moisture product with high t…
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…
Time resolved 2 million year old supernova activity discovered in Earth's microfossil record
Peter Ludwig, Shawn Bishop, Ramon Egli +11
Massive stars, which terminate their evolution as core collapse supernovae, are theoretically predicted to eject more than 1E-5 solar masses of the radioisotope 60Fe. If such an ev…