  In this work we selected one particular fibril from a high resolution solar
chromosphere observation from the Dutch Open Telescope, and tried to obtain a
broad picture of the intricate mechanism that might be incorporated in the
multiple layer of the Solar atmosphere in high cadence multi-wavelength
observation. We analyzed the changingvfibril patter using multi-wavelength
tomography, which consists of both H$\alpha$ line center \& the blue wing,
Doppler-signal, Ca II H, and the G-band. We have found that the intermittent
ejected material through fibril from Doppler images has clearly shown
oscillation mode, as seen in the H$\alpha$ blue wing. The oscillations in the
umbrae and penumbrae magnetic field lines that are above the sunspot cause a
broadening and forms the area like a ring shape from 3 to 15-minute
oscillations as function of height. These made a distinct boundary of umbrae
and penumbrae which suggest the comb structure, and indicate that the
oscillations could propagate along the inclined magnetic flux tubes from below.
The 3-minute strongly appeared in the broadly inclined penumbrae magnetic filed
lines and gave the clear light-bridge. The well known 5-minute was dominated in
the umbrae-penumbrae region boundary, the long 7-minute one was transparent in
the H$\alpha$ blue wing, but this was the same with 10 and 15-minute, it was
concentrated in the inner-penumbrae, as seen in the H$\alpha$ line center. From
these findings we propose a picture on the role of fibril as the fabric of
interaction between the layers, also the related activites around the active
region under investigation.
