  We investigate the traveling kink oscillation triggered by a solar flare on
2022 September 29. The observational data is mainly measured by the Solar Upper
Transition Region Imager (SUTRI), the Atmospheric Imaging Assembly (AIA), and
the Spectrometer/Telescope for Imaging X-rays (STIX). The transverse
oscillations with apparent decaying in amplitudes, which are nearly
perpendicular to the oscillating loop, are observed in passbands of SUTRI 465
A, AIA 171 A, and 193 A. The decaying oscillation is launched by a solar flare
erupted closely to one footpoint of coronal loops, and then it propagates along
several loops. Next, the traveling kink wave is evolved to a standing kink
oscillation. To the best of our knowledge, this is the first report of the
evolution of a traveling kink pulse to a standing kink wave along coronal
loops. The standing kink oscillation along one coronal loop has a similar
period of about 6.3 minutes at multiple wavelengths, and the decaying time is
estimated to about 9.6-10.6 minutes. Finally, two dominant periods of 5.1
minutes and 2.0 minutes are detected in another oscillating loop, suggesting
the coexistence of the fundamental and third harmonics.
