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Oscillations on Width and Intensity of Slender Ca II H Fibrils from SUNRISE/SuFI

  • Authors: R. Gafeira, S. Jafarzadeh, S. K. Solanki, A. Lagg, M. van Noort, P. Barthol, J. Blanco Rodríguez, J. C. del Toro Iniesta, A. Gandorfer, L. Gizon, J. Hirzberger, M. Knölker, D. Orozco Suárez, T. L. Riethmüller, and W. Schmidt

2017 The Astrophysical Journal Supplement Series 229 7.

  • Provider: AAS Journals

Caption: Figure 3.

Temporal variation of an SCF. The images of a straightened fibril at different times are vertically stacked. Individual images, recorded every 7 s, are separated by horizontal black lines. The vertical arrow indicates the period of the fibril’s intensity fluctuation. The color represents intensity, normalized to the mean value of the quiet region marked in Figure 1.

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