  The `blazar sequence' has been proposed for more than 20 years, yet its
nature is still unclear. In this work, for the first time, we expand this topic
to the TeV band by using a sample of 58 TeV blazars including 48 blazars in the
quiescent state and 21 blazars in the flaring state. We investigate the
correlation between the TeV luminosity, which has been compensated for
attenuation from extragalactic background light, and the synchrotron peak
frequency. We note that there is no correlation between TeV luminosity and peak
frequency in the quiescent state and a strong anti-correlation in the flaring
state for the observed value. However, there is a strong positive correlation
in both the quiescent state and the flaring state for the intrinsic value. This
indicates that the blazar sequence is shown in the flaring state rather than in
the quiescent state for the observed value and the blazar sequence is not
present in both two states after removing the beaming effect. In addition, to
confirm whether the beaming effect results in the blazar sequence, we compare
the \textit{Fermi} $\gamma$-ray luminosity between the quiescent state and the
flaring state. We find the \textit{Fermi} $\gamma$-ray luminosity in the
flaring state is greater than that in the quiescent state and the Doppler
factor in the flaring state is greater. We suggest the blazar sequence in the
flaring state may be due to the stronger beaming effect.
