activity
20152025
most citedSolar prominences: 'double, double ... boil and bubble'

44 citations · 105 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2025

Forming prominences accounting for partial ionisation effects

V. Jerčić, B. Popescu Braileanu, R. Keppens

One of the most striking structures in the solar atmosphere are prominences, predominantly coronal structures, with thermodynamic conditions that vary from chromospheric internally…

astro-ph.SR2024★ 3 cited

Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths

A. G. M. Pietrow, V. Liakh, C. M. J. Osborne +2

We present synthetic spectra corresponding to a 2.5D magnetohydrodynamical simulation of a rotating prominence in the Ca II 8542 Å, H, Ca II K, Mg II k, Ly , and Ly lines…

astro-ph.SR2024

Prominence and coronal rain formation by steady versus stochastic heating and how we can relate it to observations

V. Jerčić, J. M. Jenkins, R. Keppens

Prominences and coronal rain are two forms of coronal condensations for which we still lack satisfactory details on the formation pathways and conditions under which the two come t…

astro-ph.SR2023★ 9 cited

Two-fluid reconnection jets in a gravitationally stratified atmosphere

B. Popescu Braileanu, R. Keppens

The density decreases exponentially with height in the solar gravitationally stratified atmosphere, therefore the collisional coupling between the ionized plasma and the neutrals a…

astro-ph.SR2022★ 20 cited

1.5D NLTE spectral synthesis of a 3D filament/prominence simulation

J. M. Jenkins, C. M. J. Osborne, R. Keppens

Aims. We here demonstrate how the recently developed Lightweaver framework makes non-LTE (NLTE) spectral synthesis feasible on a new 3D ab-initio magnetohydrodynamic (MHD) filament…

astro-ph.SR2022★ 29 cited

The influence of flux rope heating models on solar prominence formation

N. Brughmans, J. M. Jenkins, R. Keppens

Aims. We begin by exploring the influence of two classes of commonly adopted heating models on the formation behaviour of solar prominences. These models consider either an exponen…

astro-ph.SR2015★ 44 cited

Solar prominences: 'double, double ... boil and bubble'

Rony Keppens, Chun Xia, Oliver Porth

Observations revealed rich dynamics within prominences, the cool 10,000 K, macroscopic (sizes of order 100 Mm) "clouds" in the million degree solar corona. Even quiescent prominenc…