  Based on the analysis of the microwave observations at frequency of 2.60 --
3.80 GHz in a solar X1.3 flare event observed at Solar Broadband
RadioSpectrometer in Huairou (SBRS/Huairou) on 2005 July 30, an interesting
reversed drifting quasi-periodic pulsating structure (R-DPS) is confirmed. The
R-DPS is mainly composed of two drifting pulsating components: one is a
relatively slow very short-period pulsation (VSP) with period of about 130 --
170 ms, the other is a relatively fast VSP with period of about 70 -- 80 ms.
The R-DPS has a weak left-handed circular polarization. Based on the synthetic
investigations of Reuven Ramaty High Energy Solar Spectroscopic Imaging
(RHESSI) hard X-ray, Geostationary Operational Environmental Satellite (GOES)
soft X-ray observation, and magnetic field extrapolation, we suggest the R-DPS
possibly reflects flaring dynamic processes of the emission source regions.
