We present Monte Carlo simulations of the Galactic population of radio and gamma-ray pulsars using the predicted luminosities of the polar cap emission model. Assuming an emission solid angle of 1 steradian and alignment of the radio and gamma-ray beams, we explore cases with and without magnetic field decay. For the case of field decay on a

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Terrestrial albedo data are important for climate model studies because of the impor- tance albedo has on the net radiation budget of the Earth. Direct measurements of the albedo are not common, and there is no dataset with global coverage that offers an alternative to data from satellite measurements. The satellite data, however, are often from