First-authored, refereed papers of Christoph Kuckein

A list of first-authored, refereed publications of Christoph Kuckein, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-3242-1497

List of publications ordered by citations
Number of papers: 11
No. of citations: 333

2025

1. Inferring chromospheric velocities in an M3.2 flare using He I 1083.0 nm and Ca II 854.2 nm [5]
   Kuckein, C., Collados, M., Asensio Ramos, A., Díaz Baso, C. J., Felipe, T., Quintero Noda, C., Kleint, L., Fletcher, L. & Matthews, S., A&A, 699, A121

2021

1. Multiple Stokes I inversions for inferring magnetic fields in the spectral range around Cr I 5782 Å [11]
   Kuckein, C., Balthasar, H., Quintero Noda, C., Diercke, A., Trelles Arjona, J. C., Ruiz Cobo, B., Felipe, T., Denker, C., Verma, M., Kontogiannis, I. & Sobotka, M., A&A, 653, A165

2020

1. Determining the dynamics and magnetic fields in He I 10830 Å during a solar filament eruption [20]
   Kuckein, C., González Manrique, S. J., Kleint, L. & Asensio Ramos, A., A&A, 640, A71

2019

1. Height variation of magnetic field and plasma flows in isolated bright points [19]
   Kuckein, Christoph, A&A, 630, A139

2017

1. Ca II 8542 Å brightenings induced by a solar microflare [7]
   Kuckein, C., Diercke, A., González Manrique, S. J., Verma, M., Löhner-Böttcher, J., Socas-Navarro, H., Balthasar, H., Sobotka, M. & Denker, C., A&A, 608, A117

2016

1. Giant quiescent solar filament observed with high-resolution spectroscopy [29]
   Kuckein, C., Verma, M. & Denker, C., A&A, 589, A84

2015

1. Magnetic and Dynamical Photospheric Disturbances Observed During an M3.2 Solar Flare [20]
   Kuckein, C., Collados, M. & Manso Sainz, R., ApJ, 799, L25

2012

1. An active region filament studied simultaneously in the chromosphere and photosphere. II. Doppler velocities [46]
   Kuckein, C., Martínez Pillet, V. & Centeno, R., A&A, 542, A112
2. An active region filament studied simultaneously in the chromosphere and photosphere. I. Magnetic structure [96]
   Kuckein, C., Martínez Pillet, V. & Centeno, R., A&A, 539, A131

2011

1. Continuous upflow of material in an active region filament from thephotosphere to the corona [0]
   Kuckein, C., Centeno, R. & Martinez Pillet, V., Highlights of Spanish Astrophysics VI (Editors: Zapatero Osorio, M. R., Gorgas, J., Maiz Apellániz, J., Pardo, J. R. & Gil de Paz, A.), p. 636

2009

1. Magnetic field strength of active region filaments [80]
   Kuckein, C., Centeno, R., Martínez Pillet, V., Casini, R., Manso Sainz, R. & Shimizu, T., A&A, 501, 1113