82 citations · 216 across the 7 of their papers we have counts for
7 papers
Heating of the solar chromosphere through current dissipation
J. M. da Silva Santos, S. Danilovic, J. Leenaarts +5
The solar chromosphere is heated to temperatures higher than predicted by radiative equilibrium. This excess heating is greater in active regions where the magnetic field is strong…
Monte Carlo characterization of PETALO, a full-body liquid xenon-based PET detector
J. Renner, C. Romo-Luque, R. J. Aliaga +24
New detector approaches in Positron Emission Tomography imaging will play an important role in reducing costs, lowering administered radiation doses, and improving overall performa…
An observationally-constrained model of strong magnetic reconnection in the solar chromosphere. Atmospheric stratification and estimates of heating rates
C. J. Díaz Baso, J. de la Cruz Rodríguez, J. Leenaarts
The evolution of the photospheric magnetic field plays a key role in the energy transport into the chromosphere and the corona. In active regions, newly emerging magnetic flux inte…
Line formation of He I D3 and He I 10830 Å in a small-scale reconnection event
T. Libbrecht, J. P. Bjørgen, J. Leenaarts +3
Aims. We aim to explain line formation of He I D3 and He I 10830 Å in small-scale reconnection events. Methods. We make use of a simulated Ellerman bomb (EB), present in a Bifrost-…
Chromospheric polarimetry through multi-line observations of the 850 nm spectral region II: A magnetic flux tube scenario
C. Quintero Noda, Y. Kato, Y. Katsukawa +10
In this publication we continue the work started in Quintero Noda et al. (2017) examining this time a numerical simulation of a magnetic flux tube concentration. Our goal is to stu…
Spectropolarimetric capabilities of Ca II 8542 A line
C. Quintero Noda, T. Shimizu, J. de la Cruz Rodríguez +4
The next generation of space and ground-based solar missions aim to study the magnetic properties of the solar chromosphere using the infrared Ca II lines and the He I 10830 Å line…