Figure 3 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Chromospheric Dynamics of an Umbral Flare Kernel—Based on Coordinated SUNRISE III SCIP and Domeless Solar Telescope Observations

Authors: Ayumi Asai, Satoru UeNo, Takuma Matsumoto, Takayoshi Oba, Yukio Katsukawa, Masahito Kubo, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Hirohisa Hara, Yoshihiro Naito, Toshifumi Shimizu, Sami K. Solanki, Andreas Lagg, Achim Gandorfer, Jose Carlos del Toro Iniesta, Pietro Bernasconi, Thomas Berkefeld, Alex Feller, Tino L. Riethmüller, Alberto Álvarez-Herrero, H. N. Smitha, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Laurent Gizon, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hoelken, Francisco A. Iglesias, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinović

Ayumi Asai et al 2026 The Astrophysical Journal Letters 1008 .

Provider: AAS Journals

Caption: Figure 3.

(a) SCIP Ca 8542 line-center image taken in the raster scan starting at 03:10:31 UT. The red dashed–dotted line indicates the position across the flare kernel where the intensity profile shown in panel (c) (top) was measured. (b) SDO/AIA 94 Å image taken at 03:16:48 UT. The purple dashed line indicates the position used to derive the intensity profiles shown in panel (c) (bottom) and the time slice image shown in panel (d). (c) Top: intensity profile across the flare kernel measured along the red line shown in panel (a). Bottom: intensity profile across the flare loop measured along the purple line shown in panel (b). The intensities are scaled arbitrarily. (d) Time slice image constructed along the purple dashed line in panel (b), showing the temporal evolution of fine structures in the flare loops.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions