Manuela Temmer
University of Graz
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0003-4867-7558
About
Manuela Temmer is since 2016 Associate Professor and head of the Heliospheric Research Group (swe.uni-graz.at) at UNI Graz. After finishing her PhD studies in 2004 at UNI Graz, several self-funded research projects (FWF Erwin Schrödinger and Elise Richter fellowship, ÖAW APART scholarship) supported her post-doc stays at the Hvar Observatory of the University of Zagreb (Croatia), the Space Research Institute of the Austrian Academy of Sciences, and the Lockheed Martin Solar and Astrophysics Laboratory in Palo Alto (USA). In 2019 she was shortlisted for the “Stanford University Distinguished Visiting Austrian Chair Professorship”. In 2024 she was nominated for the position of Director of the Department of Solar and Heliospheric Research at the Max Planck Institute for Solar System Research in Göttingen.
Her research focus lies in solar and heliospheric physics, with application to the impact of solar activity on Earth as well as human and robotic explorers across the solar system (Space Weather). She works toward understanding the physics behind the dynamic processes and interrelations between flares, coronal mass ejections, and solar wind structures in interplanetary space. Besides working in an interdisciplinary field across several physics domains, of current major interest is the validation and improvement of state-of-the-art Space Weather models by using remote sensing image data and in-situ measurements from multiple viewpoints.
Employment
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University of Graz Associate Professor2016 - Present
Education
Education history is unavailable.
Projects & Funding
Projects & funding information is unavailable.
Publications (304)
- A Study on the geoeffective event of 11 April 2022 Save
- Quantifying and modeling the storm-induced orbital decay of 11 LEO satellites during 1-14 May 2024 Save
- Comparative 3D Asymmetric Expansion and Angular-width Evolution of Fast and Slow Coronal Mass Ejections Save
- Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-duration Magnetic Field Sector Transition Save
- A view of the evolution of a coronal mass ejection and the associated wave trains at high spatial and temporal resolution Save
- Understanding the Evolution of the Three-part Structure of a Coronal Mass Ejection Using Multiviewpoint Observations Save
- Automatic Detection of Blobs in WISPR/Parker Solar Probe Data Using a Machine Learning Approach Save
- Characterisation of in situ signatures of coronal mass ejections interacting with high-speed streams Save
- Evaluating the OMNI Database: Statistical Analysis of Time-Shifted L1 Data Versus Direct Near-Earth Solar Wind Observations Save
- Inverse velocity dispersion events in multi-spacecraft analyses Save
- Investigating the evolution of erupting prominences seamlessly using mosaics of EUI/FSI and Metis Save
- P2D – A two-dimensional solar wind persistence model Save
- Solar UV flux in relation to airglow variability as seen by MATS Save
- Disruption of the October 3, 2024 CME by the Heliospheric Current Sheet – A Sun-to-Earth Analysis Save
- Tracing CME Initiation from the Low Corona to the Inner Heliosphere Save
- Persistence of Solar Wind Velocity along Radial, Longitudinal, and Latitudinal Spacecraft Separation Save
- Characterisation of in situ signatures of coronal mass ejections interacting with high-speed streams Save
- Evaluating the OMNI Database: Statistical Analysis of Time‐Shifted L1 Data Versus Direct Near‐Earth Solar Wind Observations Save
- Implementing 3D Geometry of a Coronal Mass Ejection in the Drag‐Based Model Save
- Magnetic Topology and Loop Statistics in Observed Coronal Holes Using Potential Field Modeling Save