Equivalent temperature is a measure of heat in the atmosphere that accounts for the latent heat stored in water vapor in addition to sensible heat as measured by temperature. The equivalent temperature ($T_e$) scales linearly with the moist enthalpy (i.e., the temperature and humidity) of the atmosphere. Te is computed from: $$T_e = T + \frac{L_v}{C_p} q \tag{1}$$ in which $T$ is the (dry-bulb) air temperature (Kelvin), $q$ is the specific humidity, $L_v$ is the latent heat of vaporization, $C_p$ is the specific heat capacity of air at constant pressure, and $q$ is the specific humidity. The second term on the right-hand-side of Eq. 1 therefore represents the amount of warming that an air parcel would experience if all its water vapor condensed. Unless in a completely dry atmosphere, $T_e$ is therefore always greater than $T$.

Equivalent temperature can be computed from any concurrent air temperature and specific humidity data. In practice (for near-surface values), this usually requires calculating specific humidity from air temperature, dewpoint temperature, and surface air pressure. Currently, HadISDH.land provides the state-of-the-art estimates using in situ data (Willett et al., 2014). Here, we also discuss how HadISDH.land compares with estimates from the ERA5 reanalysis. Note that in HadISDH.land, climatological surface air pressure (estimated from the nearest ERA5 1-degree grid box) is used to compute $T_e$. For ERA5, surface air pressure fields can be used directly.