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20192026
most citedStatistical Analysis and Catalog of Non-polar Coronal Holes Covering the SDO-era using CATCH

77 citations · 179 across the 8 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2026

A Self-consistent Model for the Generation of Coronal Condensations: The Effects of Turbulent Wave Dissipation

M. McMurdo, V. Jercic, T. Van Doorsselaere +1

Prominences and coronal rain are two manifestations of coronal condensations whose formation mechanisms remain only partially understood. While previous studies have explored how l…

astro-ph.SR2026

Multi-wavelength synthesis of a flux rope-trapped mini-prominence eruption and post-flare coronal rain

Samrat Sen, Alexander G. M. Pietrow, Veronika Jercic +1

Small-scale eruptive phenomena in the solar corona including miniature flux ropes and associated cool plasma condensations are not fully understood despite increasing high-resoluti…

astro-ph.SR2026

From simulations to observations of cool plasma: What we can learn from synthetic spectra

V. Jerčić, T. A. Kucera, A. G. M. Pietrow +2

Cool plasma of coronal rain or prominences and filaments is ubiquitous in the solar corona. We explored the synthetic spectra of MgII h&k lines in detail and analyse how well a non…

astro-ph.SR2025

Formation of a Coronal Hole by a quiet-Sun Filament Eruption

Stefan J. Hofmeister, Eleanna Asvestari, Karin Dissauer +9

A coronal hole formed as a result of a quiet-Sun filament eruption close to the solar disk center on 2014 June 25. We studied this formation using images from the Atmospheric Imagi…

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

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.SR2022★ 21 cited

Dynamic formation of multi-threaded prominences in arcade configurations

V. Jerčić, R. Keppens

With this study, we aim to understand the nature of prominences, governed by their formation process. We use a state-of-the-art threaded prominence model within a dipped magnetic a…

astro-ph.SR2021★ 8 cited

Multi-threaded prominence oscillations triggered by a coronal shock wave

V. Jerčić, R. Keppens, Y. Zhou

In this work, we study the causal relations between a localised energy release and a remote prominence oscillation, where the prominence has a realistic thread-like structure. We u…

astro-ph.SR2021★ 36 cited

Implementing the MULTI-VP coronal model in EUHFORIA: test case results and comparisons with the WSA coronal model

Evangelia Samara, Rui F. Pinto, Jasmina Magdalenic +6

In this study, we focus on improving EUHFORIA (European Heliospheric Forecasting Information Asset), a recently developed 3D MHD space weather prediction tool. EUHFORIA consists of…

astro-ph.SR2019★ 37 cited

A statistical study of long-term evolution of coronal hole properties as observed by SDO

Stephan G. Heinemann, Veronika Jerčić, Manuela Temmer +5

The study of the evolution of coronal holes (CHs) is especially important in the context of high-speed solar wind streams (HSS) emanating from them. Stream interaction regions may…

astro-ph.SR2019★ 77 cited

Statistical Analysis and Catalog of Non-polar Coronal Holes Covering the SDO-era using CATCH

Stephan G. Heinemann, Manuela Temmer, Niko Heinemann +5

Coronal holes are usually defined as dark structures as seen in the extreme ultraviolet and X-ray spectrum which are generally associated with open magnetic field. Deriving reliabl…