In nuclear physics, it denotes the probability that a neutron will pass a given barrier, and beryllium and lead are noted for their high values of it.
In simulations of one version of this value, the Phong-Blinn Model is transformed by its "pumping up," leading to metallic effects. The Adem Equation gives the net surface longwave radiation as a function of this value, deviation from mean temperature and the probability of entrapment. Another version of it is related by the (*) Heyney-Greenstein phase function to the single free parameter and incident angle. In nuclear physics, it denotes the probability that a neutron will pass a given barrier, and beryllium and lead are noted for their high values of it. A version of Kirchhoff's Law of Radiation defines it as 1 minus the emissivity, though its value is more often given as a ratio of scattered power to total power, and it nears its maximum value for polished silver. For 10 points, name this measure most often used in the calculation of planetary energy budgets defined as the total reflected light over the incident light.
In simulations of one version of this value, the Phong-Blinn Model is transformed by its "pumping up," leading to metallic effects.
{albedo}