Empirical relationships relating density-dependent first-year survival of pike to the density of hatched eggs were taken from Minns et al. (1996) and converted into a more common representation of a dome-shaped stock-recruitment function.
As density logs are not often run from surface, we calculated the density from the interval velocity using the relation of Gardner et al. (1974), which relates density to interval velocity, where there are no density logs.
Electronic structure calculations which are based on Wannier, like localized orbitals or the related density matrix, are an alternative to conventional calculations based on extended orbitals.
Temperature related density effects became observable for both heat and solute, as the temperature anomaly increased above 12 degrees centigrade, and affected down gradient propagation.
The formula of Gardner et al. (1974) that relates density to velocity is as follows: rho = aupsilon^{b} (7 where ρ is density, υ is velocity, and a and b are parameters.
Although our main interest is in providing a simple proof of the so-called AW integral, we will list related densities for better exposition and for indicating the ways of possible generalization of AW integrals and polynomials.
