  In this paper, we present the imaging and spectroscopic observations of the
simultaneous horizontal and vertical large-amplitude oscillation of a quiescent
filament triggered by an EUV wave on 2022 October 02. Particularly, the
filament oscillation involved winking phenomenon in Ha images and horizontal
motions in EUV images. Originally, a filament and its overlying loops across AR
13110 and 13113 erupted with a highly inclined direction, resulting in an X1.0
flare and a non-radial CME. The fast lateral expansion of loops excited an EUV
wave and the corresponding Moreton wave propagating northward. Once the EUV
wavefront arrived at the quiescent filament, the filament began to oscillate
coherently along the horizontal direction and the winking filament appeared
concurrently in Ha images. The horizontal oscillation involved an initial
amplitude of 10.2 Mm and a velocity amplitude of 46.5 km/s, lasting for 3
cycles with a period of 18.2 minutes and a damping time of 31.1 minutes. The
maximum Doppler velocities of the oscillating filament are 18 km/s (redshift)
and 24 km/s (blueshift), which was derived from the spectroscopic data provided
by CHASE/HIS. The three-dimensional velocity of the oscillation is determined
to be 50 km/s at an angle of 50 to the local photosphere plane. Based on the
wave-filament interaction, the minimum energy of the EUV wave is estimated to
be 2.7 10 20 J. Furthermore, this event provides evidence that Moreton
wavesshould be excited by the highly inclined eruptions.
