Dan Krog
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View article: A Monte Carlo approach to study the effect of ions on the nucleation of sulfuric acid–water clusters
A Monte Carlo approach to study the effect of ions on the nucleation of sulfuric acid–water clusters Open
The nucleation of sulfuric acid–water clusters is a significant contribution to the formation of aerosols as precursors of cloud condensation nuclei (CCN). Depending on the temperature, there is an interplay between the clustering of parti…
View article: Dust in brown dwarfs and extra-solar planets -3D Monte Carlo versus kinetic approach of TiO2 seed formation
Dust in brown dwarfs and extra-solar planets -3D Monte Carlo versus kinetic approach of TiO2 seed formation Open
<p>Modelling the formation of cloud condensation nuclei is key for predicting cloud properties in and analyzing observational data from exoplanet and brown dwarf atmospheres. Based on kinetic results on cloud formation in exoplanets,…
View article: Dust in brown dwarfs and extra-solar planets. VIII. TiO$_2$ seed formation: 3D Monte Carlo versus kinetic approach
Dust in brown dwarfs and extra-solar planets. VIII. TiO$_2$ seed formation: 3D Monte Carlo versus kinetic approach Open
We aim to understand the onset of cloud formation {and study the formation of} TiO$_2$-CCNs. The formation of (TiO$_2$)$_{\rm N}$ clusters as precursors to extrasolar cloud formation is modelled by two different methods in order to underst…
View article: Dust in brown dwarfs and extra-solar planets
Dust in brown dwarfs and extra-solar planets Open
Context. Modelling the formation of cloud condensation nuclei (CCNs) is key for predicting cloud properties in planet and brown dwarf atmospheres. The large diversity of exoplanets (rocky planets, mini-Neptunes, giant gas planets) requires…