Two microwave type-U bursts observed with the 2.6-3.8 GHz spectrometer of B
eijing Astronomical Observatory (BAO) are described and analysed in this pa
per. The microwave type-U bursts have very short durations (about 200 ms),
narrow bandwidth. high-frequency drift rates of the ascending and descendin
g branches, and a high degree of circular polarization (80%). The sense of
polarization remains the same from the ascending to the descending branch.