  For the 2017 September 6 flare (SOL2017-Sep-06T11:53) we present not only
unusual radio bursts, but also their interesting time association with the
other flare phenomena observed in EUV, white-light, X-ray, and $\gamma$-ray
emissions. Using our new method based on wavelets we found quasi-periodic
pulsations (QPPs) in several locations of the whole time-frequency domain of
the analyzed radio spectrum (11:55-12:07 UT and 22-5000 MHz). Among them the
drifting QPPs are new and the most interesting, especially a bi-directional QPP
at the time of the hard X-ray and $\gamma$-ray peaks, and a sunquake start. In
the pre-impulsive phase we show an unusual drifting pulsation structure (DPS)
in association with the EUV brightenings caused by the interaction of magnetic
ropes. In the flare impulsive phase we found an exceptional radio burst
drifting from 5000 MHz to 800 MHz. In connection with this drifting burst, we
show a U-burst at about the onset time of an EUV writhed structure and a
drifting radio burst as a signature of a shock wave at high frequencies
(1050-1350 MHz). In the peak flare phase we found an indication of an
additional energy-release process located at higher altitudes in the solar
atmosphere. These phenomena are interpreted considering a rising magnetic rope,
magnetosonic waves and particle beams. Using a density model we estimated the
density, wave velocities and source heights for the bi-directionally drifting
QPPs, the density for the pre-impulsive DPS and U-burst, and the density and
magnetic field strength for the drifting radio burst.
