  Temperature profiles retrieved using the first set of data of the Emirates
Mars InfraRed Spectrometer (EMIRS) obtained during the science phase of the
Emirates Mars Mission (EMM) are used for the analysis of migrating thermal
tides in the Martian atmosphere. The selected data cover a solar longitude (LS)
range of 60{\deg}-90{\deg} of Martian Year (MY) 36. The novel orbit design of
the Hope Probe leads to a good geographic and local time coverage that
significantly improves the analysis. Wave mode decomposition suggests dominant
diurnal tide and important semi-diurnal tide with maximal amplitudes of 6K and
2K, respectively, as well as the existence of ~0.5K ter-diurnal tide. The
results agree well with predictions by the Mars Planetary Climate Model (PCM),
but the observed diurnal tide has an earlier phase (3h), and the semi-diurnal
tide has an unexpectedly large wavelength (~200km).
