
petr.heinzel@uwr.edu.pl
tel. +48 71 375 75 60
Zainteresowania
- solar physics
- astronomy astrophysics
- sun
- the sun
- active sun
- solar corona
- plasma astrophysics
- sun corona
- sun corona
- solar wind
Dyscyplina naukowa
- astronomia
Najnowsze publikacje
- Coronal Heating Rate in the Slow Solar Wind
- First Metis Detection of the Helium D3 Line Polarization in a Large Eruptive Prominence
- Analysis of the Stellar Occultations during the Unprecedented Long-duration Flare
- Metis Observation of the Onset of Fully Developed Turbulence in the Solar Corona
- Recurrent solar density transients in the slow wind observed with the Metis coronagraph
- Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph
- The F-CHROMA grid of 1D RADYN flare models
- Eruptive events with exceptionally bright emission in H I Ly-α observed by the Metis coronagraph
- Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?
- Energy Budget in the Solar Corona
- First polar observations of the fast solar wind with the Metis – Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration
- In-flight radiometric calibration of the Metis Visible Light channel using stars and comparison with STEREO-A/COR2 data
- Observations and modeling of spectral line asymmetries in stellar flares
- On the Physical Nature of the so-Called Prominence Tornadoes
- The diversity of spectral shapes of hydrogen Lyman lines and Mg II lines in a quiescent prominence
- Hydrogen recombination continua in stellar flares
- Doppler dimming and brightening effects in solar prominences
- High-precision spectral inversions: Determining what is important for the accurate definition of incident radiation boundary conditions
- Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment
- First Comparison of FLARIX Simulations with MSDP Observation of the C1.6 Solar Flare in the Hα Line of Hydrogen