  We measure the spectrum of cosmic rays with energies greater than $10^{18.2}$
eV with the Fluorescence Detectors (FDs) and the Surface Detectors (SDs) of the
Telescope Array Experiment using the data taken in our first 2.3-year
observation from May 27 2008 to September 7 2010. A hybrid air shower
reconstruction technique is employed to improve accuracies in determination of
arrival directions and primary energies of cosmic rays using both FD and SD
data. The energy spectrum presented here is in agreement with our previously
published spectra and the HiRes results.
