9 citations · 9 across the 2 of their papers we have counts for
3 papers
astro-ph.SR2024
A Markovian description of the multi-level source function and its application to the Lyman series in the Sun
K. Krikova, T. M. D. Pereira
Aims. We introduce a new method to calculate and interpret indirect transition rates populating atomic levels using Markov chain theory. Indirect transition rates are essential to…
astro-ph.SR2024
Observations of magnetic reconnection in the deep solar atmosphere in the H-epsilon line
L. Rouppe van der Voort, J. Joshi, K. Krikova
Magnetic reconnection in the deep solar atmosphere can give rise to enhanced emission in the Balmer hydrogen lines, a phenomenon known as Ellerman bombs (EBs). It is most common to…
astro-ph.SR2023★ 9 cited
Formation of H in the solar atmosphere
K. Krikova, T. M. D. Pereira, L. H. M. Rouppe van der Voort
Aims. We aim to understand how Hepsilon is formed in the quiet Sun. In particular, we consider the particular physical mechanism that sets its source function and extinction, how i…