activity
20072025
most citedMagnetic loop emergence within a granule

61 citations · 734 across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.SR2025

An Unusual Velocity Field in a Sunspot Penumbra

H. Balthasar, C. Denker, A. Diercke +6

The photospheric Evershed flow is normally oriented radially outward, yet sometimes opposite velocities are observed not only in the chromosphere but also in the photospheric layer…

astro-ph.SR2024

The dependence of the magnetism of a near-limb sunspot on height

M. Benko, H. Balthasar, P. Gömöry +2

The physical parameters of the sunspot are not fully understood, especially the height dependence of the magnetic field. So far, it is also an open question as to which heights the…

astro-ph.SR2021★ 14 cited

Velocity difference of ions and neutrals in solar prominences

Eberhard Wiehr, Goetz Stellmacher, Horst Balthasar +1

Marked velocity excesses of ions relative to neutrals are obtained from two time series of the neighboring emission lines He I 5015 and Fe II 5018 in a quiescent prominence. Their…

astro-ph.SR2021★ 12 cited

Multiple Stokes I inversions to infer magnetic fields in the spectral range around Cr I 5782 Å

C. Kuckein, H. Balthasar, C. Quintero Noda +8

The spectral window, containing Fraunhofer lines formed in the solar photosphere, around the magnetically sensitive Cr I lines at 5780.9, 5781.1, 5781.7, 5783.0, and 5783.8 Å, with…

astro-ph.SR2020★ 14 cited

Classification of High-resolution Solar Hα Spectra using t-distributed Stochastic Neighbor Embedding

Meetu Verma, Gal Matijevič, Carsten Denker +7

The Hα spectral line is a well-studied absorption line revealing properties of the highly structured and dynamic solar chromosphere. Typical features with distinct spectral signatu…

astro-ph.SR2020★ 26 cited

Observational study of chromospheric heating by acoustic waves

V. Abbasvand, M. Sobotka, M. Švanda +9

Aims. To investigate the role of acoustic and magneto-acoustic waves in heating the solar chromosphere, observations in strong chromospheric lines are analyzed by comparing the dep…