In this work we continue our previous work on wave propagation analysis using multi-wavelength images from Dutch Open Telescope from exceptional data observed of Active Region 10789, 2005 July, 13th. By Fourier analysis we study the layer by layer interaction of the Solar atmosphere represented by multi-wavelength, consist of Hα both line center & the blue wing, Ca II H, and the G Band. By Fourier decomposition from power, coherence and phase-difference along the fibril we try to discuss the possible mechanism in the area under investigation.
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