activity
20232026
most citedThe GAPS programme at TNG. XLV. HI Balmer lines transmission spectroscopy and NLTE atmospheric modelling of the ultra-hot Jupiter KELT-20b/MASCARA-2b

24 citations · 40 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2026

UK White Paper on Space-based total solar eclipse observations: structure and dynamics of the solar atmosphere

Lucie M. Green, Nicola Baresi, Huw Morgan +19

Our Sun is uniquely placed to enable a detailed study of astrophysical plasmas and how they are governed by the magnetic fields that thread through them. On the one hand, magnetic…

astro-ph.SR2026

Polarimetric Tomography Applied to Synthetic Multi-Spacecraft White-Light Images: Observing Coronal Mass Ejections in 3D

David Barnes, Erika Palmerio, Tanja Amerstorfer +7

A discrete tomography method has been developed that is able to reconstruct three-dimensional coronal mass ejection (CME) density structure. We test the method by producing synthet…

astro-ph.SR2025★ 1 cited

Comparative analysis of two episodes of strongly geoeffective CME events in November and December 2023

M. Temmer, M. Dumbovic, K. Martinic +8

In autumn 2023, a series of closely timed eruptive events were observed remotely and measured in situ. We studied analogous solar events, where several CMEs were launched partly fr…

astro-ph.SR2024★ 15 cited

Internal magnetic field structures observed by PSP/WISPR in a filament related coronal mass ejection

G. M. Cappello, M. Temmer, A. Vourlidas +7

We track and investigate from white-light data taken with the Wide-field Instrument for Solar PRobe (WISPR) aboard Parker Solar Probe (PSP), localized density enhancements, reflect…

astro-ph.EP2023★ 24 cited

The GAPS programme at TNG. XLV. HI Balmer lines transmission spectroscopy and NLTE atmospheric modelling of the ultra-hot Jupiter KELT-20b/MASCARA-2b

L. Fossati, F. Biassoni, G. M. Cappello +27

We aim at extracting the transmission spectrum of the HI Balmer lines of the ultra-hot Jupiter (UHJ) KELT-20b/MASCARA-2b from observations and to further compare the results with w…