84 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Instituto de Astrofísica de CanariasES11 papers
- Johns Hopkins University Applied Physics LaboratoryUS11 papers
- Institut für SonnenphysikDE10 papers
- Instituto de Astrofísica de AndalucíaES10 papers
- Instituto Nacional de Técnica AeroespacialES10 papers
- Max Planck Institute for Solar System ResearchDE10 papers
- National Astronomical Observatory of JapanJP10 papers
- National Institute for Fusion ScienceJP10 papers
- The Graduate University for Advanced Studies, SOKENDAIJP10 papers
- The University of TokyoJP10 papers
- University of GrazAT10 papers
- Consejo Nacional de Investigaciones Científicas y TécnicasAR9 papers
28 papers
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…
Cause of chromospheric opposite polarity intrusions discovered in Sunrise III/SCIP data: MURaM-ChE simulations point to twisted flux ropes
Patrick A. Ondratschek, Damien F. Przybylski, Robert H. Cameron +33
The Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) instrument onboard the balloon-borne Sunrise III observatory provided new high-resolution observations of the solar chr…
Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by Sunrise III/SCIP
Masahito Kubo, Yukio Katsukawa, Yusuke Kawabata +38
The balloon-borne stratospheric solar observatory Sunrise III successfully completed 6.5 days of observations in July 2024. One of its focal-plane instruments, the Sunrise Chromosp…
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…
Height Dependent Phase Shifts of Wave Pulses in the Lower Solar Atmosphere Measured with SUNRISE III
Andreas Lagg, H. N. Smitha, Sami K. Solanki +32
We report on the measurement of the height-dependent time shifts of wave pulses in the lower solar atmosphere from high-resolution spectro-polarimetric observations obtained with t…
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…
Magnetically Structured Oscillatory Power Along an Active-Region Transect in Near-UV Sunrise-III/SUSI Spectroscopy
Shahin Jafarzadeh, David B. Jess, Marco Stangalini +33
We present a multi-line characterisation of how oscillatory power is organised across distinct magnetic environments in an active region using seeing-free, stratospheric near-ultra…
Multi-line Wave Signatures in a Sunspot from Near-UV Sunrise III/SUSI Observations
Shahin Jafarzadeh, David B. Jess, Marco Stangalini +32
Magnetohydrodynamic waves redistribute energy in magnetic structures of the lower solar atmosphere, yet constraints on how wave power and dominant frequencies are organised above s…
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…
A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
G. Russano, Y. De Leo, F. Frassati +13
Context. Studying the kinematic and dynamic evolution of fast eruptive events from the middle to high solar corona is a primary objective of the Metis coronagraph on Solar Orbiter.…
On the dynamics, thermodynamics and fine structure of virtual erupting filaments
Dion Donné, Yuhao Zhou, Hebe Cremades +1
It is not fully understood why some solar filaments erupt while others do not. Those that do typically undergo a slow rise followed by an acceleration phase, though this transition…
Tuneable skyrmion and anti-skyrmion fluids via mechanical strain in chiral kagome lattice
Gonzalo dos Santos, Flavia A. Gómez Albarracín, Ludovic D. C. Jaubert +3
Magnetic skyrmions are nanometric swirling spin textures that exhibit remarkable stability at finite temperatures, making them promising candidates for spintronic applications. Ach…
Automatic detection of CMEs using synthetically-trained Mask R-CNN
Francisco A. Iglesias, Diego G. Lloveras, Florencia L. Cisterna +6
Coronal mass ejections (CMEs) are a major driver of space weather. To assess CME geoeffectiveness, among other scientific goals, it is necessary to reliably identify and characteri…
Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense
Auriane Egal, Denis Vida, François Colas +94
Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmo…
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…
Quantifying errors in 3D CME parameters derived from synthetic data using white-light reconstruction techniques
Christine Verbeke, M. Leila Mays, Christina Kay +10
(Shortened version) Current efforts in space weather forecasting of CMEs have been focused on predicting their arrival time and magnetic structure. To make predictions, methods hav…
A New Approach to Sonification of Astrophysical Data: The User Centred Design of SonoUno
Johanna Casado, Beatriz García, Poshak Gandhi +1
Even when actual technologies present the potential to augment inclusion and the United Nations has been stablished the digital access to information as a human right, people with…
Distorted-Toroidal Flux Rope model for Heliospheric Flux Ropes
Teresa Nieves-Chinchilla, Miguel Angel Hidalgo, Hebe Cremades
The three-dimensional characterization of magnetic flux-ropes observed in the heliosphere has been a challenging task for decades. This is mainly due to the limitation to infer the…
Atomistic simulations of ductile failure in a b.c.c. high entropy alloy
Franco Aquistapace, Nicolás Vazquez, Matías Chiarpotti +3
Ductile failure is studied in a bcc HfNbTaZr High Entropy Alloy (HEA) with a pre-existing void. Using molecular dynamics simulations of uniaxial tensile tests, we explore the effec…
Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption
Reetika Joshi, Cristina H. Mandrini, Ramesh Chandra +5
How filaments form and erupt are topics about which solar researchers have wondered since more than a century and that are still open to debate. We present observations of a filame…
Pseudostreamer influence on flux rope evolution
A. Sahade, M. Cécere, M. V. Sieyra +3
A critical aspect of solar activity is the coupling between eruptions and the surrounding coronal magnetic field, which determines the trajectory and morphology of the eruptive eve…
A feasibility analysis towards the simulation of hysteresis with spin-lattice dynamics
G. dos Santos, F. Romá, J. Tranchida +3
We use spin-lattice dynamics simulations to study the possibility of modeling the magnetic hysteresis behavior of a ferromagnetic material. The temporal evolution of the magnetic a…
Inducing a topological transition in graphene nanoribbons superlattices by external strain
E. Flores, Jose D. Mella, E. Aparicio +4
Armchair graphene nanoribbons, when forming a superlattice, can be classified in different topological phases, with or without edge states. By means of tight-binding and classical…
Size and temperature dependent magnetization of iron nanoclusters
G. Dos Santos, R. Aparicio, D. Linares +4
The magnetic behavior of bcc iron nanoclusters, with diameters between 2 and 8 nm, is investigated by means of spin dynamics (SD) simulations coupled to molecular dynamics (MD-SD),…