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Height-dependent Phase Shifts of Wave Pulses in the Lower Solar Atmosphere Measured with SUNRISE III

  • Authors: Andreas Lagg, H. N. Smitha, Sami K. Solanki, Tino L. Riethmüller, Achim Gandorfer, Alex Feller, Francisco A. Iglesias, Azaymi L. Siu-Tapia, Jose Carlos del Toro Iniesta, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Masahito Kubo, David Orozco Suárez, Robert Cameron, Jesper Schou, Damien Przybylski, Alberto Álvarez-Herrero, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Shahin Jafarzadeh, Lakshmi Pradeep Chitta, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hölken, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Hanna Strecker, Dušan Vukadinovic

Andreas Lagg et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 5.

Height dependence of time lags for all 502 traced pulses with respect to the peak position of the deepest forming spectral line (t0). Upper left panel: the individual lines connect the time lags of a single pulse measured at the line-core formation heights of all spectral lines computed from the best-matching MHD atmosphere. The three examples shown in the bottom panel of Figure 4 are highlighted with increased opacity, with their highest point marked with a star. Upper right panel: histograms of time lags for three different height ranges. Bottom: same as the top panel, but now with the continuum intensity as the color-shading agent.

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