From the 1 of 7 papers with an AI index.
3 citations
- Institut für SonnenphysikDE6 papers
- Instituto de Astrofísica de AndalucíaES6 papers
- Instituto de Astrofísica de CanariasES6 papers
- Johns Hopkins University Applied Physics LaboratoryUS6 papers
- Max Planck Institute for Solar System ResearchDE6 papers
- National Astronomical Observatory of JapanJP6 papers
- National Institute for Fusion ScienceJP6 papers
- The Graduate University for Advanced Studies, SOKENDAIJP6 papers
- The University of TokyoJP6 papers
- University of MendozaAR6 papers
- Kanazawa UniversityJP5 papers
- Parc Científic de la Universitat de ValènciaES5 papers
7 papers
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…
Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by Sunrise III/SCIP
Masahito Kubo, Yukio Katsukawa, Yusuke Kawabata +38
The paper presents high‑precision spectropolarimetric observations of a quiet‑Sun region using the Sunrise III/SCIP instrument, revealing narrow, thread‑like chromospheric magnetic…
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…
A variational formulation of the adjoint Kutta condition in potential flow
Carlos Lozano, Jorge Ponsin
We give a variational formulation of the continuous adjoint Kutta condition for two-dimensional subcritical potential flow, with emphasis on the Kutta condition and the role of the…
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…