Diana Morosan
diana.morosan@utu.fi |
I am a researcher in the Space Research Laboratory at UTU working in the field of Solar and Space Physics. My main research interest are radio emission, plasma processes and accelerated particles associated with coronal mass ejections (CMEs) from the Sun. Radio emission on the Sun is produced by fast electrons travelling at a fraction of the speed of light. Solar radio bursts are good indicators of where particles are accelerated during solar eruptions. Studying solar eruptions and associated fast particles are of major importance since these solar phenomena can impact the near-Earth space technology, polar routes aviation and even ground-based infrastructure.
- Determining the acceleration regions of in situ electrons using remote radio and X-ray observations (2025)
- Astronomy and Astrophysics
- Fine structures of a solar type III radio bursts observed with LOFAR (2025)
- Acta Geophysica
- Imaging and spectropolarimetric observations of a band-split type II solar radio burst with LOFAR (2025)
- Astronomy and Astrophysics
- Resolving spatial and temporal shock structures using LOFAR observations of type II radio bursts (2025)
- Astronomy and Astrophysics
- The source sizes of type II radio bursts with LOFAR (2025)
- Astronomy and Astrophysics
- Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection (2024)
- Astronomy and Astrophysics
- Estimating the lateral speed of a fast shock driven by a coronal mass ejection at the location of solar radio emissions (2024)
- Astronomy and Astrophysics
- Imaging spectroscopy of a spectral bump in a type II radio burst (2024)
- Astronomy and Astrophysics
- Spatially resolved radio signatures of electron beams in a coronal shock (2024)
- Astronomy and Astrophysics
- The solar cycle 25 multi-spacecraft solar energetic particle event catalog of the SERPENTINE project (2024)
- Astronomy and Astrophysics