activity
20062025
most citedPreprocessing of vector magnetograph data for a non-linear force-free magnetic field reconstruction

432 citations · 2.9k across the 54 of their papers we have counts for

collaborators

54 papers

astro-ph.SR2025

Observing the solar corona from a formation-flying mission. First results of Proba-3/ASPIICS

A. N. Zhukov, L. Dolla, M. Mierla +32

We report the first results from observations of the solar corona by the ASPIICS coronagraph aboard the Proba-3 mission. ASPIICS (Association of Spacecraft for Polarimetric and Ima…

astro-ph.SR2025

Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun

O. Podladchikova, A. Warmuth, L. Harra +30

Small-scale impulsive energy-release events are widely considered a key ingredient of quiet-Sun coronal heating. We quantified the thermal-energy content of extreme-ultraviolet (EU…

astro-ph.SR2025★ 1 cited

The ASPIICS solar coronagraph aboard the Proba-3 formation flying mission. Scientific objectives and instrument design

A. N. Zhukov, C. Thizy, D. Galano +67

We describe the scientific objectives and instrument design of the ASPIICS coronagraph launched aboard the Proba-3 mission of the European Space Agency (ESA) on 5 December 2024. Pr…

astro-ph.SR2022★ 3 cited

Polarimetric Studies of a Fast Coronal Mass Ejection

Marilena Mierla, Bernd Inhester, Andrei N. Zhukov +4

In this work we performed a polarimetric study of a fast and wide coronal mass ejection (CME) observed on 12 July 2012 by the COR1 and COR2 instruments onboard Solar TErrestrial RE…

astro-ph.SR2022★ 8 cited

Three-dimensional analyses of an aspherical coronal mass ejection and its driven shock

Beili Ying, Li Feng, Bernd Inhester +4

Context. Observations reveal that shocks can be driven by fast coronal mass ejections (CMEs) and play essential roles in particle accelerations. A critical ratio, , derived from…

astro-ph.SR2022★ 5 cited

Coronal magnetic field evolution over the cycle 24

I. Chifu, B. Inhester, T. Wiegelmann

The photospheric magnetic field vector is continuously derived from measurements, while reconstruction of the three-dimensional (3D) coronal magnetic field requires modelling with…