  Single-pulse studies are important to understand the pulsar emission
mechanism and the noise floor in precision timing. We study total intensity and
polarimetry properties of three bright millisecond pulsars - PSRs J1022+1001,
J1713+0747, and B1855+09 - that have detectable single pulses at multiple
frequencies. We report for the first time the detection of single pulses from
PSRs J1022+1001 and J1713+0747 at 4.5 GHz. In addition, for those two pulsars
the fraction of linear polarization in the average profile is significantly
reduced at 4.5 GHz, compared to 1.38 GHz, which could support the expected
deviation from a dipolar field closer to the pulsar surface. There is a hint of
orthogonal modes in the single pulses of PSR J1713+0747. More sensitive
multi-frequency observations may be useful to confirm these findings. The
jitter noise contributions at 1.38 GHz, scaled to one hour, for PSRs
J1022+1001, J1713+0747 and B1855+09 are ~135 ns, ~45 ns, and ~60 ns
respectively and are consistent with previous studies. We also show that
selective bright-pulse timing of PSR J1022+1001 yields improved
root-mean-square residuals of ~22 $\mu$s, which is a factor of ~3 better than
timing using single pulses alone.
