most citedThe Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III

5 citations · 5 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

Three-dimensional Magnetic Structures of Ellerman Bombs revealed by SUNRISE III/SCIP

Yusuke Kawabata, Yukio Katsukawa, Masahito Kubo +37

Ellerman bombs (EBs) are widely recognized as photospheric and chromospheric signatures of magnetic reconnection. However, the three-dimensional (3D) magnetic topology has remained…

astro-ph.SR2026

Multi-height Identification of Sausage and Fluting Eigenmodes in a Solar Pore

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +34

Magnetic pores are compact, strongly magnetised waveguides in the lower solar atmosphere and therefore provide favourable conditions for identifying magnetohydrodynamic (MHD) wave…

astro-ph.SR20265 cited

The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III

Y. Katsukawa, J. C. del Toro Iniesta, S. K. Solanki +54

The Sunrise balloon-borne solar observatory is equipped with a one-meter aperture optical telescope, offering a unique platform for uninterrupted seeing-free observations across ul…

astro-ph.IM2026

Sunrise III: The Wavefront Correction System

Thomas Berkefeld, Alexander Bell, Reiner Volkmer +19

This paper describes the wave-front correction and image stabilisation system (CWS) developed for the Sunrise III balloon-borne telescope, and provides information about its perfor…

astro-ph.SR2025

The first out-of-ecliptic observations of the polar magnetic field of the Sun

D. Calchetti, S. K. Solanki, J. Hirzberger +25

Direct remote-sensing observations of the solar poles have been hindered by the restricted view obtained from the ecliptic plane. For the first time ever, Solar Orbiter with its re…

astro-ph.SR2025

Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun

L. P. Chitta, D. Calchetti, J. Hirzberger +26

Magnetoconvection at the solar surface governs the dynamics in the upper solar atmosphere and sustains the heliosphere. Properties of this fundamental process are poorly described…