  Observations of the Sun's off-limb white-light (WL) flares offer rare
opportunities to study the energy release and transport mechanisms in flare
loops. One of the best such events was SOL2017-09-10, an X8.2 flare that
occurred near the Sun's west limb on 2017 September 10 and produced a WL loop
system lasting more than 60 minutes and reaching an altitude higher than 30 Mm.
The event was well observed by a suite of ground- and space-based instruments,
including the Solar Dynamics Observatory/Helioseismic and Magnetic Imager
(SDO/HMI) that captured its off-limb loops in WL continuum near Fe I 6173 A,
and the Atmospheric Imager Assembly (SDO/AIA) that observed its ultraviolet
(UV) and extreme-ultraviolet (EUV) counterparts. We found quasi-periodic
pulsations in the WL and UV emissions at the flare loop-top with a period
around 8.0 min. Each pulsation appears to have an EUV counterpart that occurs
earlier in time and higher in altitude. Despite many similarities in the WL and
UV images and light curves, the WL flux at the loop-top continues to grow for
about 16 minutes while the UV fluxes gradually decay. We discuss the
implication of these unprecedented observations on the understanding of the
enigmatic off-limb WL flare emission mechanisms.
