activity
20232026
most citedSunrise III: Overview of Observatory and Instruments

32 citations · 57 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Episodic Plasma Flows and Coronal Brightenings in an Arch Filament System Observed with SUNRISE III

Sergio Javier González Manrique, Juan Carlos Trelles Arjona, Christoph Kuckein +43

Emerging flux regions (EFRs) transport magnetic flux and release energy in the solar atmosphere, often hosting arch filament systems (AFSs). We present high-resolution observations…

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.SR2026★ 2 cited

Solar flare ribbons structured by uncombed chromospheric loops

L. P. Chitta, E. R. Priest, David Orozco Suárez +33

A part of the magnetic energy released during a flare is transported to the lower atmosphere. High-resolution observations show that flare ribbons, sites of energy deposition at th…

astro-ph.SR2025★ 3 cited

Near-continuous tracking of solar active region NOAA 13664 over three solar rotations

I. Kontogiannis, Y. Zhu, K. Barczynski +6

Magnetic flux emergence and decay in the Sun span from days to months. However, their tracking is typically limited to about half a solar rotation when relying on single-vantage-po…

astro-ph.SR2025★ 2 cited

Magnetic properties of orphan penumbrae

J. S. Castellanos Durán, B. Löptien, A. Korpi-Lagg +2

Orphan penumbrae (OPU) are features resembling sunspot penumbrae, but are not connected to an umbra. Here we compare OPUs and sunspot penumbrae, including their filaments. We also…

astro-ph.SR2025

Transverse waves observed in a fibril with the MiHI prototype

E. Petrova, T. Van Doorsselaere, M. van Noort +2

Context. Fine-scale structures of the solar chromosphere, particularly fibrils, are known to host various types of magnetohydrodynamic (MHD) waves that can transport energy to the…

astro-ph.IM2025

The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument description

A. Feller, A. Gandorfer, B. Grauf +46

The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrentl…

astro-ph.IM2025★ 32 cited

Sunrise III: Overview of Observatory and Instruments

Andreas Korpi-Lagg, Achim Gandorfer, Sami K. Solanki +117

In July 2024, Sunrise completed its third successful science flight. The Sunrise III observatory had been upgraded significantly after the two previous successful flights in 2009 a…

astro-ph.SR2024★ 6 cited

: A spectropolarimetric inversion code for the coupled inference of atomic line parameters

D. Vukadinović, H. N. Smitha, A. Korpi-Lagg +3

For many transitions, atomic data, such as the oscillator strength (log(gf)) and the central wavelength of the line, are poorly constrained or even unknown. We present and test a n…

astro-ph.SR2024★ 5 cited

The MODEST catalog of depth-dependent spatially coupled inversions of sunspots observed by Hinode/SOT-SP

J. S. Castellanos Durán, N. Milanovic, A. Korpi-Lagg +3

We present a catalog that we named MODEST containing depth-dependent information on the atmospheric conditions inside sunspot groups of all types. The catalog is currently composed…

astro-ph.SR2023★ 7 cited

Expulsion of counter Evershed flows from sunspot penumbrae

J. S. Castellanos Durán, A. Korpi-Lagg, S. K. Solanki

In addition to the Evershed flow directed from the umbra towards the outer boundary of the sunspot, under special circumstances, a counter Evershed flow (CEF) in the opposite direc…