USE OF THE EFFECTIVE TEMPERATURE CONCEPT TO ACCOUNT FOR TEMPERATURE VARIATION IN CLUMPED ISOTOPE MEASUREMENTS OF GAR SCALES
The effective temperature is defined as the steady temperature that would produce the same Δ47 value as produced by the variable temperature experienced by the sample. The method has a long history: Pallmann et al., 1940; Lee, 1969; McCoy, 1987; Rogers, 2007; 2008. It is designed for any system where growth or production, P, is well-defined by an Arrhenius function, P ∝ exp(-Ea/RT), where Ea is the activation energy, T is temperature (K), and R is Boltzman’s constant. The surface temperature variation is usually represented by a harmonic series with a mean (annual) temperature Tm and sin functions with parameters ΔTd and ΔTs equal to the average range for daily and seasonal temperature variations (Rogers, 2007, 2008). We used the Daymet V4 climate dataset to estimate these parameters for sample locations. The temperature function is then combined with the Arrhenius function to determine an average value for P. The Metabolic Theory of Ecology (Brown et al., 2004) demonstrates that growth rates across a large range of organisms, including fish, have a fixed Ea = 60 kJ/mol. This value allows us to find Te for each of our sample locations. We find that Te is the same as Tm in the tropics, but can be 12 °C greater than Tm in mid-latitude settings. We anticipate that this approach will be useful for calibration and prediction of temperature using other geochemical methods.